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    <title>Advances in Theoretical and Mathematical Physics Articles (Project Euclid)</title>
    <link>http://projecteuclid.org/euclid.atmp</link>
    <description>The latest articles from Advances in Theoretical and Mathematical Physics on Project Euclid, a site for mathematics and statistics resources.</description>
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    <copyright>Copyright 2010 Cornell University Library</copyright>
    <webMaster>Euclid-L@cornell.edu (Project Euclid Team)</webMaster>
    <pubDate>Thu, 05 Aug 2010 15:41 EDT</pubDate>
    <lastBuildDate>Mon, 01 Nov 2010 09:46 EDT</lastBuildDate>
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      <title>Equivariant cohomology of the chiral de Rham complex and the half-twisted gauged sigma model</title>
      <link>http://projecteuclid.org/euclid.atmp/1278423128</link>
      <description>&lt;strong&gt;Meng-Chwan Tan&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 13, Number 4, 897--946.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 In this paper, we study the perturbative aspects of the half-twisted
					variant of Witten’s topological A-model coupled to a non-dynamical
					gauge field with Kähler target space X being a G-manifold. Our main
					objective is to furnish a purely physical interpretation of the equivariant
					cohomology of the chiral de Rham complex, recently constructed
					by Lian and Linshaw, called the “chiral equivariant cohomology.”
					In doing so, one finds that key mathematical results such as the vanishing
					in the chiral equivariant cohomology of positive weight classes,
					lend themselves to straightforward physical explanations. In addition,
					one can also construct topological invariants of X from the correlation
					functions of the relevant physical operators corresponding to the nonvanishing
					weight-zero classes. Via the topological invariance of these
					correlation functions, one can verify, from a purely physical perspective,
					the mathematical isomorphism between the weight-zero subspace of the
					chiral equivariant cohomology and the classical equivariant cohomology
					of X. Last but not least, one can also determine fully, the de Rham
					cohomology ring of X/G, from the topological chiral ring generated by
					the local ground operators of the physical model under study. 
			 &lt;/p&gt;</description>
      <guid isPermaLink="false">projecteuclid.org/euclid.atmp/1278423128_Thu, 05 Aug 2010 15:41 EDT</guid>
      <pubDate>Thu, 05 Aug 2010 15:41 EDT</pubDate>
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  <item><title>On the global structure of the Pomeransky–Senkov black holes</title><link>http://projecteuclid.org/euclid.atmp/1335273533</link><description>&lt;strong&gt;Piotr T. Chrúsciel&lt;/strong&gt;, &lt;strong&gt;Julien Cortier&lt;/strong&gt;, &lt;strong&gt;Alfonso García-Parrado Gómez-Lobo&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 14, Number 6, 1779--1856.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We construct analytic extensions of the Pomeransky–Senkov metrics
					with multiple Killing horizons and asymptotic regions. We show that,
					in our extensions, the singularities associated to an obstruction to differentiability
					of the metric lie beyond event horizons. We analyze the
					topology of the non-empty singular set, which turns out to be parameterdependent.
					The resulting global structure is somewhat reminiscent of
					that of Kerr space-time. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1335273533_Tue, 24 Apr 2012 09:18 EDT</guid><pubDate>Tue, 24 Apr 2012 09:18 EDT</pubDate></item><item><title>Wall-crossing of D4-branes using flow trees</title><link>http://projecteuclid.org/euclid.atmp/1335278889</link><description>&lt;strong&gt;Jan Manschot&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 1, 1--42.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 The moduli dependence of D4-branes on a Calabi–Yau manifold is
					studied using attractor flow trees, in the large volume limit of the Kähler
					cone. One of the moduli-dependent existence criteria of flow trees is the
					positivity of the flow parameters along its edges. It is shown that the sign
					of the flow parameters can be determined iteratively as function of the
					initial moduli, without explicit calculation of the flow of the moduli in
					the tree. Using this result, an indefinite quadratic form, which appears in
					the expression for the D4-D2-D0 BPS mass in the large volume limit, is
					proven to be positive definite for flow trees with 3 or less endpoints. The
					contribution of these flow trees to the BPS partition function is therefore
					convergent. From non-primitive wall crossing is deduced that the S-duality invariant partition function must be a generating function of the rational invariants
					$\bar{\Omega} (\Gamma) = \Sigma_{m|\Gamma} =\frac {\Omega(\Gamma/m)}{m^2}$ instead of the integer invariants $\Omega(\Gamma)$. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1335278889_Tue, 24 Apr 2012 10:48 EDT</guid><pubDate>Tue, 24 Apr 2012 10:48 EDT</pubDate></item><item><title>Invertible defects and isomorphisms of rational CFTs</title><link>http://projecteuclid.org/euclid.atmp/1335278890</link><description>&lt;strong&gt;Alexei Davydov&lt;/strong&gt;, &lt;strong&gt;Liang Kong&lt;/strong&gt;, &lt;strong&gt;Ingo Runkel&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 1, 43--69.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Given two two-dimensional conformal field theories, a domain wall —
					or defect line—between them is called invertible if there is another defect
					with which it fuses to the identity defect. A defect is called topological if
					it is transparent to the stress tensor. A conformal isomorphism between
					the two CFTs is a linear isomorphism between their state spaces which
					preserves the stress tensor and is compatible with the operator product
					expansion. We show that for rational CFTs there is a one-to-one
					correspondence between invertible topological defects and conformal isomorphisms
					if both preserve the rational symmetry. This correspondence
					is compatible with composition. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1335278890_Tue, 24 Apr 2012 10:48 EDT</guid><pubDate>Tue, 24 Apr 2012 10:48 EDT</pubDate></item><item><title>Supersymmetric surface operators, four-manifold theory and invariants in various dimensions</title><link>http://projecteuclid.org/euclid.atmp/1335278891</link><description>&lt;strong&gt;Meng-Chwan Tan&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 1, 71--129.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We continue our program initiated in "Integration over the u-plane in Donaldson theory with surface
					operators," J. High Energy Phys. 05 (2011), to consider supersymmetric surface operators in a topologically twisted ${\cal N}=2$ pure ${\it SU}(2)$ gauge theory,
					and apply them to the study of four-manifolds and related invariants. Elegant physical proofs of various seminal theorems in four-manifold theory obtained by
					Ozsáth and Szabó and Taubes, will be furnished. In particular, we will show that Taubes’ groundbreaking and difficult result — that the ordinary SW
					invariants are in fact the Gromov invariants which count pseudo-holomorphic curves embedded in a symplectic four-manifold $X$ — nonetheless lends itself
					to a simple and concrete physical derivation in the presence of “ordinary” surface operators. As an offshoot, we will be led to several interesting and mathematically
					novel identities among the Gromov and “ramified” SW invariants of $X$, which in certain cases, also involve the instanton and monopole Floer homologies
					of its three-submanifold. Via these identities, and a physical formulation of the “ramified” Donaldson invariants of four-manifolds with boundaries, we will uncover
					completely new and economical ways of deriving and understanding various important mathematical results concerning (i) knot homology groups from “ramified”
					instantons by Kronheimer and Mrowka; and (ii) monopole Floer homology and SW theory on symplectic four-manifolds by Kutluhan–Taubes.
					Supersymmetry, as well as other physical concepts such as $R$-invariance, electric–magnetic duality, spontaneous gauge symmetry breaking and localization
					onto supersymmetric configurations in topologically twisted quantum field theories, play a pivotal role in our story. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1335278891_Tue, 24 Apr 2012 10:48 EDT</guid><pubDate>Tue, 24 Apr 2012 10:48 EDT</pubDate></item><item><title>Non-Kähler heterotic rotations</title><link>http://projecteuclid.org/euclid.atmp/1335278892</link><description>&lt;strong&gt;Dario Martelli&lt;/strong&gt;, &lt;strong&gt;James Sparks&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 1, 131--174.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We study a supersymmetry-preserving solution-generating method in heterotic supergravity. In particular, we use this method to construct one-parameter non-Kähler deformations
					of Calabi–Yau manifolds with a $U(1)$ isometry, in which the complex structure remains invariant. We explain how to obtain corresponding solutions to heterotic string theory, up
					to first order in $\alpha'$, by a modified form of the standard embedding. In the course of the paper we also show that Abelian heterotic supergravity embeds
					into type II supergravity, and note that the solution-generating method in this context is related to a dipole-type deformation when there is a field theory dual. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1335278892_Tue, 24 Apr 2012 10:48 EDT</guid><pubDate>Tue, 24 Apr 2012 10:48 EDT</pubDate></item><item><title>Stable causality of the Pomeransky–Senkov black holes</title><link>http://projecteuclid.org/euclid.atmp/1335278893</link><description>&lt;strong&gt;Piotr T. Chrúsciel&lt;/strong&gt;, &lt;strong&gt;Sebastian J. Szybka&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 1, 175--178.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We show stable causality of the Pomeransky–Senkov black rings. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1335278893_Tue, 24 Apr 2012 10:48 EDT</guid><pubDate>Tue, 24 Apr 2012 10:48 EDT</pubDate></item><item><title>Two-dimensional topological field theories as taffy</title><link>http://projecteuclid.org/euclid.atmp/1335278894</link><description>&lt;strong&gt;Matt Ando&lt;/strong&gt;, &lt;strong&gt;Eric Sharpe&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 1, 179--244.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 In this paper, we use trivial defects to define global taffy-like operations
					on string worldsheets, which preserve the field theory. We fold
					open and closed strings on a space $X$ into open strings on products of
					multiple copies of $X$, and perform checks that the “taffy-folded” worldsheets
					have the same massless spectra and other properties as the original
					worldsheets. Such folding tricks are a standard method in the defects
					community; the novelty of this paper lies in deriving mathematical identities
					to check that e.g., massless spectra are invariant in topological
					field theories. We discuss the case of the B model extensively, and also
					derive the same identities for string topology, where they become statements
					of homotopy invariance. We outline analogous results in the A
					model, B-twisted Landau–Ginzburg models, and physical strings. We
					also discuss the understanding of the closed string states as the Hochschild
					homology of the open string algebra, and outline possible applications
					to elliptic genera. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1335278894_Tue, 24 Apr 2012 10:48 EDT</guid><pubDate>Tue, 24 Apr 2012 10:48 EDT</pubDate></item><item><title>Compact supersymmetric solutions of the heterotic equations of motion in dimensions 7 and 8</title><link>http://projecteuclid.org/euclid.atmp/1337951924</link><description>&lt;strong&gt;Marisa Fernández&lt;/strong&gt;, &lt;strong&gt;Stefan Ivanov&lt;/strong&gt;, &lt;strong&gt;Luis Ugarte&lt;/strong&gt;, &lt;strong&gt;Raquel Villacampa&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 2, 245--284.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We construct explicit compact solutions with non-zero field strength,
					non-flat instanton and constant dilaton to the heterotic string equations
					in dimensions 7 and 8. We present a quadratic condition on the curvature,
					which is necessary and sufficient the heterotic supersymmetry and
					the anomaly cancellation to imply the heterotic equations of motion in
					dimensions 7 and 8. We show that some of our examples are compact
					supersymmetric solutions of the heterotic equations of motion in dimensions
					7 and 8. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1337951924_Fri, 25 May 2012 09:18 EDT</guid><pubDate>Fri, 25 May 2012 09:18 EDT</pubDate></item><item><title>The diffeomorphism supergroup of a finite-dimensional supermanifold</title><link>http://projecteuclid.org/euclid.atmp/1337951925</link><description>&lt;strong&gt;C. Sachse&lt;/strong&gt;, &lt;strong&gt;C. Wockel&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 2, 285--323.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Using the categorical description of supergeometry we give an explicit
					construction of the diffeomorphism supergroup of a compact finitedimensional
					supermanifold. The construction provides the diffeomorphism
					supergroup with the structure of a Fréchet supermanifold. In addition,
					we derive results about the structure of diffeomorphism supergroups. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1337951925_Fri, 25 May 2012 09:18 EDT</guid><pubDate>Fri, 25 May 2012 09:18 EDT</pubDate></item><item><title>String universality in six	dimensions</title><link>http://projecteuclid.org/euclid.atmp/1337951926</link><description>&lt;strong&gt;Vijay Kumar&lt;/strong&gt;, &lt;strong&gt;Washington Taylor&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 2, 325--353.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 In six dimensions, cancellation of gauge, gravitational, and mixed
					anomalies strongly constrains the set of quantum field theories, which
					can be coupled consistently to gravity. We show that for some classes of
					six-dimensional (6D) supersymmetric gauge theories coupled to gravity,
					the anomaly cancellation conditions are equivalent to tadpole cancellation
					and other constraints on the matter content of heterotic/type I compactifications
					on K3. In these cases, all consistent 6D supergravity theories
					have a realization in string theory. We find one example that may arise
					from a novel string compactification, and we identify a new infinite family
					of models satisfying anomaly factorization. We find, however, that
					this infinite family of models, as well as other infinite families of models
					previously identified by Schwarz are pathological. We suggest that it may
					be feasible to demonstrate that there is a string theoretic realization of
					all consistent 6D supergravity theories which have Lagrangian descriptions
					with arbitrary gauge and matter content. We attempt to frame this
					hypothesis of string universality as a concrete conjecture. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1337951926_Fri, 25 May 2012 09:18 EDT</guid><pubDate>Fri, 25 May 2012 09:18 EDT</pubDate></item><item><title>Rigorous construction and Hadamard property of the Unruh state in Schwarzschild spacetime</title><link>http://projecteuclid.org/euclid.atmp/1337951927</link><description>&lt;strong&gt;Claudio Dappiaggi&lt;/strong&gt;, &lt;strong&gt;Valter Moretti&lt;/strong&gt;, &lt;strong&gt;Nicola Pinamonti&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 2, 355--447.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 The discovery of the radiation properties of black holes prompted
					the search for a natural candidate quantum ground state for a massless
					scalar field theory on Schwarzschild spacetime, here considered in
					the Eddington–Finkelstein representation. Among the several available
					proposals in the literature, an important physical role is played by the
					so-called Unruh state, which is supposed to be appropriate to capture
					the physics of a black hole formed by spherically symmetric collapsing
					matter. Within this respect, we shall consider a massless Klein–Gordon
					field and we shall rigorously and globally construct such state, that is on
					the algebra of Weyl observables localised in the union of the static external
					region, the future event horizon and the non-static black hole region.
					Eventually, out of a careful use of microlocal techniques, we prove that
					the built state fulfils, where defined, the so-called Hadamard condition;
					hence, it is perturbatively stable, in other words realizing the natural
					candidate with which one could study purely quantum phenomena such
					as the role of the back reaction of Hawking’s radiation. 
				 From a geometrical point of view, we shall make a profitable use of
					a bulk-to-boundary reconstruction technique which carefully exploits the
					Killing horizon structure as well as the conformal asymptotic behaviour of
					the underlying background. From an analytical point of view, our tools
					will range from Hörmander’s theorem on propagation of singularities,
					results on the role of passive states, and a detailed use of the recently
					discovered peeling behaviour of the solutions of the wave equation in
					Schwarzschild spacetime. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1337951927_Fri, 25 May 2012 09:18 EDT</guid><pubDate>Fri, 25 May 2012 09:18 EDT</pubDate></item><item><title>Cyclotron braid group approach to Laughlin correlations</title><link>http://projecteuclid.org/euclid.atmp/1337951928</link><description>&lt;strong&gt;Janusz Jacak&lt;/strong&gt;, &lt;strong&gt;Ireneusz Jóźwiak&lt;/strong&gt;, &lt;strong&gt;Lucjan Jacak&lt;/strong&gt;, &lt;strong&gt;Konrad Wieczorek&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 2, 449--469.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Homotopy braid group description including cyclotron motion of
					charged interacting two-dimensional (2D) particles at strong magnetic
					field presence is developed in order to explain, in algebraic topology
					terms, Laughlin correlations in fractional quantum Hall systems. There
					are introduced special cyclotron braid subgroups of a full braid group
					with 1D unitary representations suitable to satisfy Laughlin correlation
					requirements. In this way an implementation of composite fermions
					(fermions with auxiliary flux quanta attached in order to reproduce
					Laughlin correlations) is formulated within uniform for all 2D particles
					braid group approach. The fictitious fluxes — vortices attached to the
					composite fermions in a traditional formulation are replaced with additional
					cyclotron trajectory loops unavoidably occurring when ordinary
					cyclotron radius is too short in comparison to particle separation and
					does not allow for particle interchanges along single-loop cyclotron braids.
					Additional loops enhance the effective cyclotron radius and restore particle
					interchanges. A new type of 2D particles — composite anyons is
					also defined via unitary representations of cyclotron braid subgroups.
					It is demonstrated that composite fermions and composite anyons are
					rightful 2D particles, not auxiliary compositions with fictitious fluxes and
					are associated with cyclotron braid subgroups instead of the full braid
					group, which may open also a new opportunity for non-Abelian composite
					anyons for topological quantum information processing applications,
					due to richer representations of subgroup than of a group. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1337951928_Fri, 25 May 2012 09:18 EDT</guid><pubDate>Fri, 25 May 2012 09:18 EDT</pubDate></item><item><title>Quantization of the Hitchin moduli spaces, Liouville theory and the geometric Langlands correspondence I</title><link>http://projecteuclid.org/euclid.atmp/1337951929</link><description>&lt;strong&gt;J. Teschner&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 2, 471--564.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We discuss the relation between Liouville theory and the Hitchin integrable
					system, which can be seen in two ways as a two step process
					involving quantization and hyperkähler rotation. The modular duality
					of Liouville theory and the relation between Liouville theory and the
					SL(2)-WZNW-model give a new perspective on the geometric Langlands
					correspondence and on its relation to conformal field theory. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1337951929_Fri, 25 May 2012 09:18 EDT</guid><pubDate>Fri, 25 May 2012 09:18 EDT</pubDate></item><item><title>The quantum chiral Minkowski and conformal superspaces</title><link>http://projecteuclid.org/euclid.atmp/1337951930</link><description>&lt;strong&gt;Dalia Cervantes&lt;/strong&gt;, &lt;strong&gt;Rita Fioresi&lt;/strong&gt;, &lt;strong&gt;María A. Lledó&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 2, 565--620.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We give a quantum deformation of the chiral super Minkowski space
					in four dimensions as the big cell inside a quantum super Grassmannian.
					The quantization is performed in such way that the actions of the
					Poincar´e and conformal quantum supergroups on the quantum Minkowski
					and quantum conformal superspaces are preserved. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1337951930_Fri, 25 May 2012 09:18 EDT</guid><pubDate>Fri, 25 May 2012 09:18 EDT</pubDate></item><item><title>Bundle gerbes for orientifold sigma models</title><link>http://projecteuclid.org/euclid.atmp/1339374265</link><description>&lt;strong&gt;Krzysztof Gawędzki&lt;/strong&gt;, &lt;strong&gt;Rafał R. Suszek&lt;/strong&gt;, &lt;strong&gt;Konrad Waldorf&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 3, 621--687.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Bundle gerbes with connection and their modules play an important
					role in the theory of two-dimensional sigma models with a background
					Wess–Zumino flux: their holonomy determines the contribution of the
					flux to the Feynman amplitudes of classical fields. We discuss additional
					structures on bundle gerbes and gerbe modules needed in similar
					constructions for orientifold sigma models describing closed and open
					strings. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339374265_Sun, 10 Jun 2012 20:24 EDT</guid><pubDate>Sun, 10 Jun 2012 20:24 EDT</pubDate></item><item><title>Decoupling gravity in F-theory</title><link>http://projecteuclid.org/euclid.atmp/1339374266</link><description>&lt;strong&gt;Clay Córdova&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 3, 689--740.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We study seven-brane SU(5) GUT models of string phenomenology
					which can be consistently analyzed in a purely local framework. The
					requirement that gravity can decouple constrains the form of four-dimensional
					physics as well as the geometry of spacetime. We rule out
					a large family of candidate UV completions of such models and derive
					a priori constraints on the local singularities of compact elliptic Calabi–
					Yau four-folds. These constraints are strong enough to obstruct a wide
					class of brane constructions from UV completion in string theory. It is
					demonstrated that consistent local models always have exotic Yukawa
					coupling structures, and hidden sectors or interesting non-perturbative
					superpotentials which merit further investigation. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339374266_Sun, 10 Jun 2012 20:24 EDT</guid><pubDate>Sun, 10 Jun 2012 20:24 EDT</pubDate></item><item><title>Superstring field theory in the democratic picture</title><link>http://projecteuclid.org/euclid.atmp/1339374267</link><description>&lt;strong&gt;Michael Kroyter&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 3, 741--781.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We present a new open superstring field theory, whose string fields
					carry an arbitrary picture number and reside in the large Hilbert space.
					The redundancy related to picture number is resolved by treating picture
					changing as a gauge transformation. A mid-point insertion is imperative
					for this formalism. We find that this mid-point insertion must include all
					multi-picture-changing operators. It is also proven that this insertion as
					well as all the multi-picture-changing operators are zero weight conformal
					primaries. This new theory solves the problems with the Ramond sector
					shared by other Ramond-Neveu-Schwarz (RNS) string field theories,
					while naturally unifying the Neveu-Schwarz (NS) and Ramond string
					fields. When partially gauge fixed, it reduces in the NS sector to the
					modified cubic superstring field theory. Hence, it shares all the good
					properties of this theory, e.g., it has analytical vacuum and marginal
					deformation solutions. Treating the redundant gauge symmetry using
					the Batalin-Vilkovisky (BV) formalism is straightforward and results in
					a cubic action with a single string field, whose quantum numbers are
					unconstrained. The generalization to an arbitrary brane system is simple
					and includes the standard Chan–Paton factors and the most general
					string field consistent with the brane system. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339374267_Sun, 10 Jun 2012 20:24 EDT</guid><pubDate>Sun, 10 Jun 2012 20:24 EDT</pubDate></item><item><title>On a possible approach to general field theories with nonpolynomial interactions</title><link>http://projecteuclid.org/euclid.atmp/1339374268</link><description>&lt;strong&gt;Franco Ferrari&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 3, 783--799.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 In this work, a class of field theories with self-interactions described by
					a potential of the kind $V (\phi(x) − \phi(x_0))$ is studied. $\phi$ is a massive scalar
					field and $x$, $x_0$ are points in a $d$-dimensional space. Under the condition
					that the potential admits the Fourier representation, it is shown that
					such theories may be mapped into a standard field theory, in which the
					interaction of the new fields is a polynomial of fourth degree. With some
					restrictions, this mapping allows the perturbative treatment of models
					that are otherwise intractable with standard field theoretical methods.
					A nonperturbative approach to these theories is attempted. The original
					scalar field $\phi$ is integrated out exactly at the price of introducing
					auxiliary vector fields. The latter are treated in a mean field theory
					approximation. The singularities that arise after the elimination of the
					auxiliary fields are cured using the dimensional regularization. The expression
					of the counterterms to be subtracted is computed. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339374268_Sun, 10 Jun 2012 20:24 EDT</guid><pubDate>Sun, 10 Jun 2012 20:24 EDT</pubDate></item><item><title>Large-spin asymptotics of Euclidean LQG flat-space wavefunctions</title><link>http://projecteuclid.org/euclid.atmp/1339374269</link><description>&lt;strong&gt;Aleksandar Miković&lt;/strong&gt;, &lt;strong&gt;Marko Vojinović&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 3, 801--847.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We analyze the large-spin asymptotics of a class of spin-network
					wavefunctions of Euclidean loop quantum gravity, which corresponds to
					a flat spacetime. A wavefunction from this class can be represented as a
					sum over the spins of an amplitude for a spin network whose graph is
					a composition of the wavefunction spin network graph with the dual
					one-complex graph and the tetrahedron graphs for a triangulation of the
					spatial 3-manifold. This spin-network amplitude can be represented as a
					product of $6j$ symbols, which is then used to find the large-spin asymptotics
					of the wavefunction. By using the Laplace method we show that
					the large-spin asymptotics is given by a sum of Gaussian functions. However,
					these Gaussian functions are not of the type, which gives the correct
					graviton propagator. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339374269_Sun, 10 Jun 2012 20:24 EDT</guid><pubDate>Sun, 10 Jun 2012 20:24 EDT</pubDate></item><item><title>D-branes, surface operators, and ADHM quiver representations</title><link>http://projecteuclid.org/euclid.atmp/1339374270</link><description>&lt;strong&gt;Ugo Bruzzo&lt;/strong&gt;, &lt;strong&gt;Wu-Yen Chuang&lt;/strong&gt;, &lt;strong&gt;Duiliu-Emanuel Diaconescu&lt;/strong&gt;, &lt;strong&gt;Marcos Jardim&lt;/strong&gt;, &lt;strong&gt;G. Pan&lt;/strong&gt;, &lt;strong&gt;Yi Zhang&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 3, 849--911.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 A supersymmetric quantum mechanical model is constructed for BPS
					states bound to surface operators in five dimensional $SU(r)$ gauge theories
					using D-brane engineering. This model represents the effective action of a
					certain D2-brane configuration, and is naturally obtained by dimensional reduction of a quiver (0, 2) gauged linear sigma model. In a special
					stability chamber, the resulting moduli space of quiver representations
					is shown to be smooth and isomorphic to a moduli space of framed quotients
					on the projective plane. A precise conjecture relating a K-theoretic
					partition function of this moduli space to refined open-string invariants
					of toric Lagrangian branes is formulated for conifold and local $\mathbb{P}^1 \times \mathbb{P}^1$
					geometries. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339374270_Sun, 10 Jun 2012 20:24 EDT</guid><pubDate>Sun, 10 Jun 2012 20:24 EDT</pubDate></item><item><title>Perturbative study of the transfer matrix on the string worldsheet in ${\rm AdS}^5 \times S_5$</title><link>http://projecteuclid.org/euclid.atmp/1339438348</link><description>&lt;strong&gt;Andrei Mikhailov&lt;/strong&gt;, &lt;strong&gt;Sakura Schäfer-Nameki&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 4, 913--971.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Quantum non-local charges are central to the quantum integrability of
					a sigma model. In this paper we study the quantum consistency and UV
					finiteness of non-local charges of string theory in ${\rm AdS}^5 \times S_5$. We use the
					pure spinor formalism. We develop the near-flat space expansion of the
					transfer matrix and calculate the one-loop divergences. We find that
					the logarithmic divergences cancel at the level of one loop. This gives
					strong support to the quantum integrability of the full string theory. We
					develop a calculational setup for the renormalization group analysis of
					Wilson line type of operators on the string worldsheet. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339438348_Mon, 11 Jun 2012 14:12 EDT</guid><pubDate>Mon, 11 Jun 2012 14:12 EDT</pubDate></item><item><title>Classification of free actions on complete intersections of four quadrics</title><link>http://projecteuclid.org/euclid.atmp/1339438349</link><description>&lt;strong&gt;Zheng Hua&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 4, 973--990.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 In this paper we classify all free actions of finite groups on Calabi–Yau
					complete intersection of four quadrics in $\mathbb{P}^7$, up to projective equivalence.
					We get some examples of smooth Calabi–Yau three-folds with large nonabelian
					fundamental groups. We also observe the relation between some
					of these examples and moduli of polarized abelian surfaces. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339438349_Mon, 11 Jun 2012 14:12 EDT</guid><pubDate>Mon, 11 Jun 2012 14:12 EDT</pubDate></item><item><title>On the final definition of the causal boundary and its relation with the conformal boundary</title><link>http://projecteuclid.org/euclid.atmp/1339438350</link><description>&lt;strong&gt;José Luis Flores&lt;/strong&gt;, &lt;strong&gt;Jónatan Herrera&lt;/strong&gt;, &lt;strong&gt;Miguel Sánchez&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 4, 991--1057.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 The notion of causal boundary $\partial M$ for a strongly causal spacetime
					$M$ has been a controversial topic along last decades: on one hand, some
					attempted definitions were not fully consistent, on the other, there were
					simple examples where an open conformal embedding $i : M \hookrightarrow M_0$ could
					be defined, but the corresponding conformal boundary $\partial_i M$ disagreed
					drastically with the causal one. Nevertheless, the recent progress in this
					topic suggests that a final option for $\partial M$ is available in most cases. Our
					study has two parts: 
				 (I) To give general arguments on a boundary in order to ensure that
					it is admissible as a causal boundary at the three natural levels, i.e., as
					a point set, as a chronological space and as a topological space. Then,
					the essential uniqueness of our choice is stressed, and the relatively few
					admissible alternatives are discussed. 
				 (II) To analyze the role of the conformal boundary $\partial_i M$. We show that,
						in general, $\partial_i M$ may present a very undesirable structure. Nevertheless, it is well behaved under certain general assumptions, and its accessible
						part $\partial^*_i M$ agrees with the causal boundary. 
				 This study justifies both boundaries. On one hand, the conformal
					boundary $\partial^*_i M$, which cannot be defined for a general spacetime but is
					easily computed in particular examples, appears now as a special case
					of the causal boundary. On the other, the new redefinition of the causal
					boundary not only is free of inconsistencies and applicable to any strongly
					causal spacetime, but also recovers the expected structure in the cases
					where a natural simple conformal boundary is available. The cases of
					globally hyperbolic spacetimes and asymptotically conformally flat ends
					are especially studied. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339438350_Mon, 11 Jun 2012 14:12 EDT</guid><pubDate>Mon, 11 Jun 2012 14:12 EDT</pubDate></item><item><title>Lie crossed modules and gauge-invariant actions for 2-BF theories</title><link>http://projecteuclid.org/euclid.atmp/1339438351</link><description>&lt;strong&gt;João Martins&lt;/strong&gt;, &lt;strong&gt;Aleksandar Miković&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 4, 1059--1084.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We generalize the BF theory action to the case of a general Lie crossed
					module $(\partial : H \to G, \triangleright)$, where $G$ and $H$ are non-abelian Lie groups. Our
					construction requires the existence of $G$-invariant non-degenerate bilinear
					forms on the Lie algebras of $G$ and $H$ and we show that there are
					many examples of such Lie crossed modules by using the construction of
					crossed modules provided by short chain complexes of vector spaces. We
					also generalize this construction to an arbitrary chain complex of vector
					spaces, of finite type. We construct two gauge-invariant actions for 2-flat
					and fake-flat 2-connections with auxiliary fields. The first action is of the
					same type as the BFCG action introduced by Girelli, Pfeiffer and Popescu
					for a special class of Lie crossed modules, where $H$ is abelian. The second action is 
					an extended BFCG action which contains an additional auxiliary
					field. However, these two actions are related by a field redefinition.
					We also construct a three-parameter deformation of the extended BFCG
					action, which we believe to be relevant for the construction of non-trivial
					invariants of knotted surfaces embedded in the four-sphere. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339438351_Mon, 11 Jun 2012 14:12 EDT</guid><pubDate>Mon, 11 Jun 2012 14:12 EDT</pubDate></item><item><title>Null asymptotics of solutions of	the Einstein–Maxwell equations in general relativity and gravitational radiation</title><link>http://projecteuclid.org/euclid.atmp/1339438352</link><description>&lt;strong&gt;Lydia Bieri&lt;/strong&gt;, &lt;strong&gt;PoNing Chen&lt;/strong&gt;, &lt;strong&gt;Shing-Tung Yau&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 4, 1085--1113.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We prove that for spacetimes solving the Einstein–Maxwell (EM) equations,
					the electromagnetic field contributes at highest order to the nonlinear
					memory effect of gravitational waves. In Nonlinear nature of gravitation and gravitational-wave
						experiments, Christodoulou showed
					that gravitational waves have a nonlinear memory. He discussed how this
					effect can be measured as a permanent displacement of test masses in a
					laser interferometer gravitational-wave detector. Christodoulou derived a
					precise formula for this permanent displacement in the Einstein vacuum
					(EV) case. We prove in Theorem 2.6 that for the EM equations this permanent
					displacement exhibits a term coming from the electromagnetic
					field. This term is at the same highest order as the purely gravitational term that governs the EV situation. On the other hand, in Section 3, we
					show that to leading order, the presence of the electromagnetic field does
					not change the instantaneous displacement of the test masses. Following
					the method introduced by Christodoulou in Nonlinear nature of gravitation and gravitational-wave
						experiments, and asymptotics derived
					by Zipser in The global nonlinear stability of the trivial solution of the
						Einstein–Maxwell equations and Extensions of the stability theorem of the Minkowski space in
							general relativity: Solutions of the Einstein–Maxwell equations , we investigate gravitational radiation at null infinity
					in spacetimes solving the EM equations. We study the Bondi mass loss
					formula at null infinity derived in Extensions of the stability theorem of the Minkowski space in
						general relativity: Solutions of the Einstein–Maxwell equations . We show that the mass loss formula
					from Extensions of the stability theorem of the Minkowski space in
						general relativity: Solutions of the Einstein–Maxwell equations is compatible with the one in Bondi coordinates obtained in Gravitational waves in general relativity X:
							Asymptotic expansions for the Einstein–Maxwell field .
					And we observe that the presence of the electromagnetic field increases
					the total energy radiated to infinity up to leading order. Moreover, we
					compute the limit of the area radius at null infinity in Theorem 2.7. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339438352_Mon, 11 Jun 2012 14:12 EDT</guid><pubDate>Mon, 11 Jun 2012 14:12 EDT</pubDate></item><item><title>Plane-symmetric spacetimes with positive cosmological constant: The case of stiff fluids</title><link>http://projecteuclid.org/euclid.atmp/1339438353</link><description>&lt;strong&gt;Philippe G. LeFloch&lt;/strong&gt;, &lt;strong&gt;Sophonie B. Tchapnda&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 4, 1115--1140.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We consider plane-symmetric spacetimes satisfying Einstein’s field
					equations with positive cosmological constant, when the matter is a fluid
					whose pressure is equal to its mass-energy density (i.e., a so-called stiff
					fluid). We study the initial-value problem for the associated Einstein
					equations and establish a global existence result. The late-time asymptotics
					of solutions is also rigorously derived, and we conclude that the
					spacetime approaches the de Sitter spacetime while the matter disperses
					asymptotically. A technical difficulty dealt with here lies in the fact that
					solutions may contain vacuum states as well as velocities approaching
					the speed of light, both possibilities leading to singular behavior in the
					evolution equations. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339438353_Mon, 11 Jun 2012 14:12 EDT</guid><pubDate>Mon, 11 Jun 2012 14:12 EDT</pubDate></item><item><title>Sums over topological sectors and
				quantization of Fayet–Iliopoulos
				parameters</title><link>http://projecteuclid.org/euclid.atmp/1339438354</link><description>&lt;strong&gt;Simeon Hellerman&lt;/strong&gt;, &lt;strong&gt;Eric Sharpe&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 4, 1141--1199.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 In this paper we discuss quantization of the Fayet–Iliopoulos parameter
					in supergravity theories with altered nonperturbative sectors, which
					were recently used to argue a fractional quantization condition. Nonlinear
					sigma models with altered nonperturbative sectors are the same as
					nonlinear sigma models on special stacks known as gerbes. After reviewing
					the existing results on such theories in two dimensions, we discuss
					examples of gerby moduli “spaces” appearing in four-dimensional field
					theory and string compactifications, and the effect of various dualities.
					We discuss global topological defects arising when a field or string theory
					moduli space has a gerbe structure. We also outline how to generalize the
					results of Bagger–Witten and more recent authors on quantization issues
					in supergravities from smooth moduli spaces to smooth moduli stacks,
					focusing particular attention on stacks that have gerbe structures. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1339438354_Mon, 11 Jun 2012 14:12 EDT</guid><pubDate>Mon, 11 Jun 2012 14:12 EDT</pubDate></item><item><title>The $n$-point functions for intersection numbers on moduli spaces of curves</title><link>http://projecteuclid.org/euclid.atmp/1349879109</link><description>&lt;strong&gt;Kefeng Liu&lt;/strong&gt;, &lt;strong&gt;Hao Xu&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 5, 1201--1236.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Using the celebrated Witten–Kontsevich theorem, we prove a recursive
					formula of the $n$-point functions for intersection numbers on moduli
					spaces of curves. It has been used to prove the Faber intersection number
					conjecture and motivated us to find some conjectural vanishing identities
					for Gromov–Witten invariants. The latter has been proved recently by
					Liu and Pandharipande. We also give a combinatorial interpretation of
					$n$-point functions in terms of summation over binary trees. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1349879109_Wed, 10 Oct 2012 10:25 EDT</guid><pubDate>Wed, 10 Oct 2012 10:25 EDT</pubDate></item><item><title>Model building with $F$-theory</title><link>http://projecteuclid.org/euclid.atmp/1349879110</link><description>&lt;strong&gt;Ron Donagi&lt;/strong&gt;, &lt;strong&gt;Martijn Wijnholt&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 5, 1237--1317.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Despite much recent progress in model building with $D$-branes, it
					has been problematic to find a completely convincing explanation of
					gauge coupling unification. We extend the class of models by considering
					$F$-theory compactifications, which may incorporate unification more
					naturally. We explain how to derive the charged chiral spectrum and
					Yukawa couplings in $N = 1$ compactifications of $F$-theory with $G$-flux.
					In a class of models which admit perturbative heterotic duals, we show
					that the $F$-theory and heterotic computations match. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1349879110_Wed, 10 Oct 2012 10:25 EDT</guid><pubDate>Wed, 10 Oct 2012 10:25 EDT</pubDate></item><item><title>Symmetries of massless vertex operators in $AdS_5 × S^5$</title><link>http://projecteuclid.org/euclid.atmp/1349879111</link><description>&lt;strong&gt;Andrei Mikhailov&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 5, 1319--1372.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 The worldsheet sigma-model of the superstring in $AdS_5 × S^5$ has a
					one-parameter family of flat connections parametrized by the spectral
					parameter. The corresponding Wilson line is not BRST invariant for
					an open contour, because the BRST transformation leads to boundary
					terms. These boundary terms define a cohomological complex associated
					to the endpoint of the contour. We study the cohomology of this complex
					for Wilson lines in some infinite-dimensional representations. We find
					that for these representations the cohomology is nontrivial at the ghost
					number 2. This implies that it is possible to define a BRST invariant
					open Wilson line. The central point in the construction is the existence
					of massless vertex operators transforming exactly covariantly under the
					action of the global symmetry group. In flat space massless vertices
					transform covariantly only up to adding BRST exact terms. But in AdS
					we show that it is possible to define vertices so that they transform exactly
					covariantly. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1349879111_Wed, 10 Oct 2012 10:25 EDT</guid><pubDate>Wed, 10 Oct 2012 10:25 EDT</pubDate></item><item><title>Division algebras and supersymmetry II</title><link>http://projecteuclid.org/euclid.atmp/1349879112</link><description>&lt;strong&gt;John C. Baez&lt;/strong&gt;, &lt;strong&gt;John Huerta&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 5, 1373--1410.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Starting from the four normed division algebras — the real numbers,
					complex numbers, quaternions and octonions — a systematic procedure
					gives a 3-cocycle on the Poincaré Lie superalgebra in dimensions 3, 4,
					6 and 10. A related procedure gives a 4-cocycle on the Poincaré Lie
					superalgebra in dimensions 4, 5, 7 and 11. In general, an$ (n + 1)$-cocycle
					on a Lie superalgebra yields a “Lie $n$-superalgebra”: that is, roughly
					speaking, an $n$-term chain complex equipped with a bracket satisfying
					the axioms of a Lie superalgebra up to chain homotopy. We thus obtain
					Lie 2-superalgebras extending the Poincaré superalgebra in dimensions
					3, 4, 6 and 10, and Lie 3-superalgebras extending the Poincaré superalgebra
					in dimensions 4, 5, 7 and 11. As shown in Sati, Schreiber and
					Stasheff’s work on higher gauge theory, Lie 2-superalgebra connections
					describe the parallel transport of strings, while Lie 3-superalgebra connections
					describe the parallel transport of 2-branes. Moreover, in the
					octonionic case, these connections concisely summarize the fields appearing
					in 10- and 11-dimensional supergravity. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1349879112_Wed, 10 Oct 2012 10:25 EDT</guid><pubDate>Wed, 10 Oct 2012 10:25 EDT</pubDate></item><item><title>Ricci-flow-conjugated initial data sets for Einstein equations</title><link>http://projecteuclid.org/euclid.atmp/1349879113</link><description>&lt;strong&gt;Mauro Carfora&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 5, 1411--1484.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We discuss a natural form of Ricci-flow conjugation between two distinct
					general relativistic data sets given on a compact $n \ge 3$-dimensional
					manifold $\Sigma$. We establish the existence of the relevant entropy functionals
					for the matter and geometrical variables, their monotonicity properties,
					and the associated convergence in the appropriate sense. We show that
					in such a framework there is a natural mode expansion generated by
					the spectral resolution of the Ricci conjugate Hodge–DeRham operator.
					This mode expansion allows one to compare the two distinct data sets
					and gives rise to a computable heat kernel expansion of the fluctuations
					among the fields defining the data. In particular, this shows that Ricciflow
					conjugation entails a natural form of $L^2$ parabolic averaging of one
					data set with respect to the other with a number of desirable properties:
					(i) It preserves the dominant energy condition; (ii) It is localized by a
					heat kernel whose support sets the scale of averaging; (iii) It is characterized
					by a set of balance functionals, that allow the analysis of its entropic
					stability. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1349879113_Wed, 10 Oct 2012 10:25 EDT</guid><pubDate>Wed, 10 Oct 2012 10:25 EDT</pubDate></item><item><title>Super Yangian of superstring on $\mathrm{AdS}_5 × S^5$ revisited</title><link>http://projecteuclid.org/euclid.atmp/1349879114</link><description>&lt;strong&gt;Machiko Hatsuda&lt;/strong&gt;, &lt;strong&gt;Kentaroh Yoshida&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 5, 1485--1501.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We construct infinite number of conserved nonlocal charges for type
					IIB superstring on the $\mathrm{AdS}_5×S^5$ space in the conformal gauge without
					assuming any $\kappa$ gauge fixing, and show that they satisfy the super
					Yangian algebra. The resultant algebra is the same as our previous work, where a special gauge was assumed in such a way that the Noether
					current satisfies a flatness condition. However the flatness condition for
					the Noether current of a superstring on the AdS space is broken in general.
					We show that the anomalous contribution is absorbed into the current
					where fermionic constraints play an essential role, and a resultant
					conserved nonlocal charge has different expression satisfying the same
					super Yangian algebra. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1349879114_Wed, 10 Oct 2012 10:25 EDT</guid><pubDate>Wed, 10 Oct 2012 10:25 EDT</pubDate></item><item><title>Hermitian–Einstein connections on polystable parabolic principal Higgs bundles</title><link>http://projecteuclid.org/euclid.atmp/1349879115</link><description>&lt;strong&gt;Indranil Biswas&lt;/strong&gt;, &lt;strong&gt;Matthias Stemmler&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 5, 1503--1521.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Given a smooth complex projective variety $X$ and a smooth divisor
					$D$ on $X$, we prove the existence of Hermitian–Einstein connections, with
					respect to a Poincaré-type metric on $X \setminus D$, on polystable parabolic principal
					Higgs bundles with parabolic structure over $D$, satisfying certain
					conditions on their restriction to $D$. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1349879115_Wed, 10 Oct 2012 10:25 EDT</guid><pubDate>Wed, 10 Oct 2012 10:25 EDT</pubDate></item><item><title>Breaking GUT groups in $F$-theory</title><link>http://projecteuclid.org/euclid.atmp/1355321968</link><description>&lt;strong&gt;Ron Donagi&lt;/strong&gt;, &lt;strong&gt;Martijn Wijnholt&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 6, 1523--1603.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We consider the possibility of breaking the GUT group to the Standard
					Model gauge group in $F$-theory compactifications by turning on certain
					$U(1)$ fluxes. We show that the requirement of massless hypercharge is
					equivalent to a topological constraint on the UV completion of the local
					model. The possibility of this mechanism is intrinsic to $F$-theory. We
					address some of the phenomenological signatures of this scenario. We
					show that our models predict monopoles as in conventional GUT models.
					We discuss in detail the leading threshold corrections to the gauge kinetic
					terms and their effect on unification. They turn out to be related to
					Ray–Singer torsion. We also discuss the issue of proton decay in $F$-theory
					models and explain how to engineer models which satisfy current
					experimental bounds. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1355321968_Wed, 12 Dec 2012 09:19 EST</guid><pubDate>Wed, 12 Dec 2012 09:19 EST</pubDate></item><item><title>$E_7$ groups from octonionic magic square</title><link>http://projecteuclid.org/euclid.atmp/1355321969</link><description>&lt;strong&gt;Sergio L. Cacciatori&lt;/strong&gt;, &lt;strong&gt;Francesco Dalla Piazza&lt;/strong&gt;, &lt;strong&gt;Antonio Scotti&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 6, 1605--1654.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 In this paper, we continue our program, started in Euler angles for $G(2)$ , of building
					up explicit generalized Euler angle parameterizations for all exceptional
					compact Lie groups. Here we solve the problem for $E_7$, by first providing
					explicit matrix realizations of the Tits construction of a Magic Square
					product between the exceptional octonionic algebra $\mathfrak{J}$ and the quaternionic
					algebra $\mathbb{H}$, both in the adjoint and the 56-dimensional representations.
					Then, we provide the Euler parametrization of $E_7$ starting from its
					maximal subgroup $U = (E_6 \times U(1))/\mathbb{Z}_3$. Next, we give the constructions
					for all the other maximal compact subgroups. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1355321969_Wed, 12 Dec 2012 09:19 EST</guid><pubDate>Wed, 12 Dec 2012 09:19 EST</pubDate></item><item><title>Riemann–Hilbert approach to the time-dependent generalized sine kernel</title><link>http://projecteuclid.org/euclid.atmp/1355321970</link><description>&lt;strong&gt;Karol Kajetan Kozlowski&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 6, 1655--1743.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We derive the leading asymptotic behavior and build a new series
					representation for the Fredholm determinant of integrable integral operators
					appearing in the representation of the time and distance-dependent
					correlation functions of integrable models described by a six-vertex
					$R$-matrix. This series representation opens a systematic way for the
					computation of the long-time, long-distance asymptotic expansion for
					the correlation functions of the aforementioned integrable models away 
					from their free fermion point. Our method builds on a Riemann–Hilbert
					based analysis. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1355321970_Wed, 12 Dec 2012 09:19 EST</guid><pubDate>Wed, 12 Dec 2012 09:19 EST</pubDate></item><item><title>A rigid Calabi–Yau three-fold</title><link>http://projecteuclid.org/euclid.atmp/1355321971</link><description>&lt;strong&gt;Sara Angela Filippini&lt;/strong&gt;, &lt;strong&gt;Alice Garbagnati&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 6, 1745--1787.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 The aim of this paper is to analyze some geometric properties of the
					rigid Calabi–Yau three-fold $\mathcal{Z}$ obtained by a quotient of $E_3$, where $E$ is a
					specific elliptic curve. We describe the cohomology of $\mathcal{Z}$ and give a simple
					formula for the trilinear form on $\mathrm{Pic}(\mathcal{Z})$. We describe some projective
					models of $\mathcal{Z}$ and relate these to its generalized mirror. A smoothing of
					a singular model is a Calabi–Yau three-fold with small Hodge numbers
					which was not known before. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1355321971_Wed, 12 Dec 2012 09:19 EST</guid><pubDate>Wed, 12 Dec 2012 09:19 EST</pubDate></item><item><title>The wave equation in a general spherically symmetric black hole geometry</title><link>http://projecteuclid.org/euclid.atmp/1355321972</link><description>&lt;strong&gt;Matthew Masarik&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 6, 1789--1815.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We consider the Cauchy problem for the wave equation in a general
					class of spherically symmetric black hole geometries. Under certain mild
					conditions on the far-field decay and the singularity, we show that there
					is a unique globally smooth solution to the Cauchy problem for the wave
					equation with data compactly supported away from the horizon that is
					compactly supported for all times and decays in $L_{loc}^\infty$ as $t$ tends to infinity .
					We obtain as a corollary that in the geometry of black hole solutions of
					the SU(2) Einstein/Yang–Mills equations, solutions to the wave equation
					with compactly supported initial data decay as $t$ goes to infinity. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1355321972_Wed, 12 Dec 2012 09:19 EST</guid><pubDate>Wed, 12 Dec 2012 09:19 EST</pubDate></item><item><title>Algebraic deformations of toric varieties II: noncommutative instantons</title><link>http://projecteuclid.org/euclid.atmp/1355321973</link><description>&lt;strong&gt;Lucio Cirio&lt;/strong&gt;, &lt;strong&gt;Giovanni Landi&lt;/strong&gt;, &lt;strong&gt;Richard J. Szabo&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 6, 1817--1907.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We continue our study of the noncommutative algebraic and differential
					geometry of a particular class of deformations of toric varieties,
					focusing on aspects pertinent to the construction and enumeration of
					noncommutative instantons on these varieties. We develop a noncommutative
					version of twistor theory, which introduces a new example of a noncommutative
					four-sphere. We develop a braided version of the ADHM
					construction and show that it parameterizes a certain moduli space of
					framed torsion free sheaves on a noncommutative projective plane. We
					use these constructions to explicitly build instanton gauge bundles with
					canonical connections on the noncommutative four-sphere that satisfy
					appropriate anti-selfduality equations. We construct projective moduli
					spaces for the torsion free sheaves and demonstrate that they are smooth.
					We define equivariant partition functions of these moduli spaces, finding
					that they coincide with the usual instanton partition functions for supersymmetric
					gauge theories on $\mathbb{C}2$. 					
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1355321973_Wed, 12 Dec 2012 09:19 EST</guid><pubDate>Wed, 12 Dec 2012 09:19 EST</pubDate></item><item><title>Codes and supersymmetry in one dimension</title><link>http://projecteuclid.org/euclid.atmp/1355321974</link><description>&lt;strong&gt;Charles F. Doran&lt;/strong&gt;, &lt;strong&gt;Michael G. Faux&lt;/strong&gt;, &lt;strong&gt;Sylvester James Gates&lt;/strong&gt;, &lt;strong&gt;Tristan Hübsch&lt;/strong&gt;, &lt;strong&gt;Kevin M. Iga&lt;/strong&gt;, &lt;strong&gt;Gregory D. Landweber&lt;/strong&gt;, &lt;strong&gt;Robert L. Miller&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 15, Number 6, 1909--1970.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Adinkras are diagrams that describe many useful supermultiplets in
					$D = 1$ dimensions. We show that the topology of the Adinkra is uniquely
					determined by a doubly even code. Conversely, every doubly even code
					produces a possible topology of an Adinkra. A computation of doubly
					even codes results in an enumeration of these Adinkra topologies up to
					$N = 28$, and for minimal supermultiplets, up to $N = 32$. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1355321974_Wed, 12 Dec 2012 09:19 EST</guid><pubDate>Wed, 12 Dec 2012 09:19 EST</pubDate></item><item><title>Chiral algebras of (0, 2) models</title><link>http://projecteuclid.org/euclid.atmp/1358950849</link><description>&lt;strong&gt;Junya Yagi&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 1, 1--37.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We explore two-dimensional sigma models with (0, 2) supersymmetry
					through their chiral algebras. Perturbatively, the chiral algebras of
					(0, 2) models have a rich infinite-dimensional structure described by the
					cohomology of a sheaf of chiral differential operators. Nonperturbatively,
					instantons can deform this structure drastically. We show that under
					some conditions they even annihilate the whole algebra, thereby triggering
					the spontaneous breaking of supersymmetry. For a certain class
					of Kähler manifolds, this suggests that there are no harmonic spinors on
					their loop spaces and gives a physical proof of the Höhn–Stolz conjecture. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950849_Wed, 23 Jan 2013 09:20 EST</guid><pubDate>Wed, 23 Jan 2013 09:20 EST</pubDate></item><item><title>Hamiltonian structure of gauge-invariant variational problems</title><link>http://projecteuclid.org/euclid.atmp/1358950850</link><description>&lt;strong&gt;Marco Castrillón López&lt;/strong&gt;, &lt;strong&gt;Jamie Muñoz Masqué&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 1, 39--63.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Let $C \to M$ be the bundle of connections of a principal bundle on $M$.
					The solutions to Hamilton–Cartan equations for a gauge-invariant
					Lagrangian density $\Lambda$ on $C$ satisfying a weak condition of regularity, are
					shown to admit an affine fibre-bundle structure over the set of solutions
					to Euler–Lagrange equations for $\Lambda$. This structure is also studied for the
					Jacobi fields and for the moduli space of extremals. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950850_Wed, 23 Jan 2013 09:20 EST</guid><pubDate>Wed, 23 Jan 2013 09:20 EST</pubDate></item><item><title>A master solution of the quantum Yang–Baxter equation and classical discrete integrable equations</title><link>http://projecteuclid.org/euclid.atmp/1358950851</link><description>&lt;strong&gt;Vladimir V. Bazhanov&lt;/strong&gt;, &lt;strong&gt;Sergey M. Sergeev&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 1, 65--95.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We obtain a new solution of the star–triangle relation with positive
					Boltzmann weights, which contains as special cases all continuous and
					discrete spin solutions of this relation, that were previously known. This
					new master solution defines an exactly solvable two lattice model of statistical
					mechanics, which involves continuous spin variables, living on a
					circle, and contains two temperature-like parameters. If one of the these
					parameters approaches a root of unity (corresponds to zero temperature),
					the spin variables freezes into discrete positions, equidistantly spaced on
					the circle. An absolute orientation of these positions on the circle slowly
					changes between lattice sites by overall rotations. Allowed configurations
					of these rotations are described by classical discrete integrable equations,
					closely related to the famous $Q_4$-equations by Adler, Bobenko and Suris.
					Fluctuations between degenerate ground states in the vicinity of zero
					temperature are described by a rather general integrable lattice model
					with discrete spin variables. In some simple special cases, the latter
					reduces to the Kashiwara–Miwa and chiral Potts models. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950851_Wed, 23 Jan 2013 09:20 EST</guid><pubDate>Wed, 23 Jan 2013 09:20 EST</pubDate></item><item><title>Modular realizations of hyperbolic Weyl groups</title><link>http://projecteuclid.org/euclid.atmp/1358950852</link><description>&lt;strong&gt;Axel Kleinschmidt&lt;/strong&gt;, &lt;strong&gt;Hermann Nicolai&lt;/strong&gt;, &lt;strong&gt;Jakob Palmkvist&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 1, 97--148.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We study the recently discovered isomorphisms between hyperbolic
					Weyl groups and modular groups over integer domains in normed division
					algebras. We show how to realize the group action via fractional
					linear transformations on generalized upper half-planes over the division
					algebras, focusing on the cases involving quaternions and octonions. For
					these we construct automorphic forms, whose explicit expressions depend
					crucially on the underlying arithmetic properties of the integer domains.
					Another main new result is the explicit octavian realization of $W+(E_{10})$,
					which contains as a special case a new realization of $W+(E_8)$ in terms of
					unit octavians and their automorphism group. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950852_Wed, 23 Jan 2013 09:20 EST</guid><pubDate>Wed, 23 Jan 2013 09:20 EST</pubDate></item><item><title>Čech cocycles for differential characteristic classes: an ∞-Lie theoretic construction</title><link>http://projecteuclid.org/euclid.atmp/1358950853</link><description>&lt;strong&gt;Domenico Fiorenza&lt;/strong&gt;, &lt;strong&gt;Urs Schreiber&lt;/strong&gt;, &lt;strong&gt;Jim Stasheff&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 1, 149--250.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 What are called secondary characteristic classes in Chern–Weil theory
					are a refinement of ordinary characteristic classes of principal bundles
					from cohomology to differential cohomology. We consider the problem of
					refining the construction of secondary characteristic classes from cohomology
					sets to cocycle spaces; and from Lie groups to higher connected
					covers of Lie groups by smooth $\infty$-groups, i.e., by smooth groupal $A_\infty$-
					spaces. Namely, we realize differential characteristic classes as morphisms
					from $\infty$-groupoids of smooth principal $\infty$-bundles with connections to
					$\infty$-groupoids of higher $U(1)$-gerbes with connections. This allows us to
					study the homotopy fibres of the differential characteristic maps thus
					obtained and to show how these describe differential obstruction problems.
					This applies in particular to the higher twisted differential spin
					structures called twisted differential string structures and twisted differential fivebrane structures . 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950853_Wed, 23 Jan 2013 09:20 EST</guid><pubDate>Wed, 23 Jan 2013 09:20 EST</pubDate></item><item><title>Old issues and linear sigma models</title><link>http://projecteuclid.org/euclid.atmp/1358950854</link><description>&lt;strong&gt;Jock McOrist&lt;/strong&gt;, &lt;strong&gt;Ilarion V. Melnikov&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 1, 251--288.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Using mirror symmetry, we resolve an old puzzle in the linear sigma
					model description of the spacetime Higgs mechanism in a heterotic string
					compactification with (2,2) worldsheet supersymmetry. The resolution
					has a nice spacetime interpretation via the normalization of physical fields
					and suggests that with a little care deformations of the linear sigma model
					can describe heterotic Higgs branches. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950854_Wed, 23 Jan 2013 09:20 EST</guid><pubDate>Wed, 23 Jan 2013 09:20 EST</pubDate></item><item><title>Equivariant modular categories via Dijkgraaf–Witten theory</title><link>http://projecteuclid.org/euclid.atmp/1358950855</link><description>&lt;strong&gt;Jennifer Maier&lt;/strong&gt;, &lt;strong&gt;Thomas Nikolaus&lt;/strong&gt;, &lt;strong&gt;Christoph Schweigert&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 1, 289--358.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Based on a weak action of a finite group $J$ on a finite group $G$, we
					present a geometric construction of $J$-equivariant Dijkgraaf–Witten theory
					as an extended topological field theory. The construction yields an
					explicitly accessible class of equivariant modular tensor categories. For
					the action of a group $J$ on a group $G$, the category is described as the representation
					category of a $J$-ribbon algebra that generalizes the Drinfel’d
					double of the finite group $G$. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950855_Wed, 23 Jan 2013 09:20 EST</guid><pubDate>Wed, 23 Jan 2013 09:20 EST</pubDate></item><item><title>The fast Newtonian limit for perfect fluids</title><link>http://projecteuclid.org/euclid.atmp/1358950885</link><description>&lt;strong&gt;Todd A. Oliynyk&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 2, 359--391.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We prove the existence of a large class of dynamical solutions to the
					Einstein–Euler equations for which the fluid density and spatial three-velocity
					converge to a solution of the Poisson–Euler equations of Newtonian
					gravity. The results presented here generalize those of The Newtonian limit for perfect fluids to allow
					for a larger class of initial data. As in The Newtonian limit for perfect fluids , the proof is based on a nonlocal
					symmetric hyperbolic formulation of the Einstein–Euler equations,
					which contain a singular parameter $\epsilon = v_T /c$ with $v_T$ a characteristic
					speed associated to the fluid and $c$ the speed of light. Energy and dispersive
					estimates on weighted Sobolev spaces are the main technical tools
					used to analyze the solutions in the singular limit $\epsilon \searrow 0$. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950885_Wed, 23 Jan 2013 09:21 EST</guid><pubDate>Wed, 23 Jan 2013 09:21 EST</pubDate></item><item><title>An extension of Friedmann–Robertson–Walker theory beyond big bang</title><link>http://projecteuclid.org/euclid.atmp/1358950886</link><description>&lt;strong&gt;Joachim Schröter&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 2, 393--419.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 Starting from the classic Friedmann–Robertson–Walker theory with
					big bang it is shown that the solutions of the field equations can be
					extended to negative times. Choosing a new cosmic time scale instead of
					proper time one achieves complete differentiability of the scale factor and
					of suitable thermodynamic quantities equivalent to pressure and energy
					density. Then, the singularity of big bang manifests itself only by the
					vanishing of the scale factor at time zero. Moreover, all solutions of the
					field equations are defined for all times from $-\infty$ to $+\infty$. In a separate
					section, the horizon structure of the extended theory is studied. Some
					weak assumptions guarantee that there are no horizons. Hence, the horizon
					problem in a strict sense disappears. An intensive discussion of the
					results is given at the end of the paper. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950886_Wed, 23 Jan 2013 09:21 EST</guid><pubDate>Wed, 23 Jan 2013 09:21 EST</pubDate></item><item><title>Higher genus BMN correlators: factorization and recursion relations</title><link>http://projecteuclid.org/euclid.atmp/1358950887</link><description>&lt;strong&gt;Min–xin Huang&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 2, 421--503.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We systematically study the factorization and recursion relations in
					higher genus correlation functions of Berenstein–Maldacena–Nastase
					(BMN) operators in free $\mathcal{N} = 4$ super Yang–Mills theory. These properties
					were found in a previous paper by the author, and were conjectured to
					result from the correspondence with type IIB string theory on the infinitely
					curved pp-wave background, where the strings become effectively
					infinitely long. Here we push the calculations to higher genus, provide
					more clarifications and verifications of the factorization and recursion
					relations. Our calculations provide conjectural indirect tests of the AdS/
					CFT correspondence for multi-loop superstring amplitudes of stringy
					modes. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950887_Wed, 23 Jan 2013 09:21 EST</guid><pubDate>Wed, 23 Jan 2013 09:21 EST</pubDate></item><item><title>Generalized TKNN-equations</title><link>http://projecteuclid.org/euclid.atmp/1358950888</link><description>&lt;strong&gt;Giuseppe De Nittis&lt;/strong&gt;, &lt;strong&gt;Giovanni Landi&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 2, 505--547.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We derive generalized TKNN-equations via bundle representations of
					the noncommutative torus with rational deformation parameter, the bundle
					coming from spectral projections in the torus algebra. These equations
					relate Chern numbers of dual bundles, which we interpret as Hall
					conductances for Dirac-like Hamiltonians describing magnetic Bloch electrons
					in a strong magnetic field. We also present their generalizations for
					irrational values of the deformation parameter. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950888_Wed, 23 Jan 2013 09:21 EST</guid><pubDate>Wed, 23 Jan 2013 09:21 EST</pubDate></item><item><title>Geometry of fractional spaces</title><link>http://projecteuclid.org/euclid.atmp/1358950889</link><description>&lt;strong&gt;Gianluca Calcagni&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 2, 549--644.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We introduce fractional flat space, described by a continuous geometry
					with constant non-integer Hausdorff and spectral dimensions. This is the
					analogue of Euclidean space, but with anomalous scaling and diffusion
					properties. The basic tool is fractional calculus, which is cast in a way
					convenient for the definition of the differential structure, distances, volumes,
					and symmetries. By an extensive use of concepts and techniques
					of fractal geometry, we clarify the relation between fractional calculus
					and fractals, showing that fractional spaces can be regarded as fractals
					when the ratio of their Hausdorff and spectral dimension is greater than
					one. All the results are analytic and constitute the foundation for field
					theories living on multi-fractal spacetimes, which are presented in a companion
					paper. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950889_Wed, 23 Jan 2013 09:21 EST</guid><pubDate>Wed, 23 Jan 2013 09:21 EST</pubDate></item><item><title>Causal posets, loops and the construction of nets of local algebras for QFT</title><link>http://projecteuclid.org/euclid.atmp/1358950890</link><description>&lt;strong&gt;Fabio Ciolli&lt;/strong&gt;, &lt;strong&gt;Giuseppe Ruzzi&lt;/strong&gt;, &lt;strong&gt;Ezio Vasselli&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 2, 645--691.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 We provide a model independent construction of a net of $C*$-algebras
					satisfying the Haag–Kastler axioms over any spacetime manifold. Such a
					net, called the net of causal loops , is constructed by selecting a suitable
					base $K$ encoding causal and symmetry properties of the spacetime. Considering
					$K$ as a partially ordered set (poset) with respect to the inclusion
					order relation, we define groups of closed paths (loops) formed by the
					elements of $K$. These groups come equipped with a causal disjointness
					relation and an action of the symmetry group of the spacetime. In this
					way, the local algebras of the net are the group $C*$-algebras of the groups
					of loops, quotiented by the causal disjointness relation. We also provide a
					geometric interpretation of a class of representations of this net in terms
					of causal and covariant connections of the poset K. In the case of the
					Minkowski spacetime, we prove the existence of Poincaré covariant representations
					satisfying the spectrum condition. This is obtained by virtue
					of a remarkable feature of our construction: any Hermitian scalar quantum
					field defines causal and covariant connections of $K$. Similar results
					hold for the chiral spacetime $S^1$ with conformal symmetry. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950890_Wed, 23 Jan 2013 09:21 EST</guid><pubDate>Wed, 23 Jan 2013 09:21 EST</pubDate></item><item><title>Persistence of gaps in the spectrum of certain almost periodic operators</title><link>http://projecteuclid.org/euclid.atmp/1358950891</link><description>&lt;strong&gt;Norbert Riedel&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 2, 693--712.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 It is shown that for any irrational rotation number and any admissible
					gap labelling number the almost Mathieu operator (also known as
					Harper’s operator) has a gap in its spectrum with that labelling number.
					This answers the strong version of the so-called "Ten Martini Problem".
					When specialized to the particular case where the coupling constant is
					equal to one, it follows that the "Hofstadter butterfly" has for any quantum
					Hall conductance the exact number of components prescribed by the
					recursive scheme to build this fractal structure. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950891_Wed, 23 Jan 2013 09:21 EST</guid><pubDate>Wed, 23 Jan 2013 09:21 EST</pubDate></item><item><title>Vortex equation and reflexive sheaves</title><link>http://projecteuclid.org/euclid.atmp/1358950892</link><description>&lt;strong&gt;Indranil Biswas&lt;/strong&gt;, &lt;strong&gt;Matthias Stemmler&lt;/strong&gt;&lt;p&gt;&lt;strong&gt;Source: &lt;/strong&gt;Adv. Theor. Math. Phys., Volume 16, Number 2, 713--723.&lt;/p&gt;&lt;p&gt;&lt;strong&gt;Abstract:&lt;/strong&gt;&lt;br/&gt; 
				 It is known that given a stable holomorphic pair $(E,\phi)$, where $E$ is a
					holomorphic vector bundle on a compact Kähler manifold $X$ and $\phi$ is a
					holomorphic section of $E$, the vector bundle $E$ admits a Hermitian metric
					solving the vortex equation. We generalize this to pairs $(E,\phi)$, where $E$
					is a reflexive sheaf on $X$. 
			 &lt;/p&gt;</description><guid isPermaLink="false">projecteuclid.org/euclid.atmp/1358950892_Wed, 23 Jan 2013 09:21 EST</guid><pubDate>Wed, 23 Jan 2013 09:21 EST</pubDate></item></channel>
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