# High Energy Physics - Theory

## New submissions

[ total of 42 entries: 1-42 ]
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### New submissions for Thu, 23 Nov 17

[1]
Title: A matrix CFT at multiple large charges
Authors: Orestis Loukas
Subjects: High Energy Physics - Theory (hep-th)

We investigate matrix models in three dimensions where the global $\text{SU}(N)$ symmetry acts via the adjoint map. Analyzing their ground state which is homogeneous in space and can carry either a unique or multiple fixed charges, we show the existence of at least two distinct fixed points of the renormalization group (RG) flow. In particular, the one type of those fixed points manifests itself via tractable deviations in the large-charge expansion from the known predictions in the literature. We demonstrate most of the novel features using mainly the example of the $\text{SU}(4)$ matrix theory to compute the anomalous dimension of the lowest scalar operator with large global charge(s).

[2]
Title: Unimodular Gravity and General Relativity UV divergent contributions to the scattering of massive scalar particles
Subjects: High Energy Physics - Theory (hep-th)

We work out the one-loop and order $\kappa^2 m_\phi^2$ UV divergent contributions, coming from Unimodular Gravity and General Relativity, to the S matrix element of the scattering process $\phi + \phi\rightarrow \phi + \phi$ in a $\lambda \phi^4$ theory with mass $m_\phi$. We show that both Unimodular Gravity and General Relativity give rise to the same UV divergent contributions in Dimension Regularization. This seems to be at odds with the known result that in a multiplicative MS dimensional regularization scheme the General Relativity corrections, in the de Donder gauge, to the beta function $\beta_{\lambda}$ of the $\lambda$ coupling do not vanish, whereas the Unimodular Gravity corrections, in a certain gauge, do vanish. Actually, we show that the UV divergent contributions to the 1PI Feynman diagrams which give rise to those non-vanishing corrections to $\beta_{\lambda}$ do not contribute to the UV divergent behaviour of the S matrix element of $\phi + \phi\rightarrow \phi + \phi$ and this shows that any physical consequence --such existence of asymptotic freedom due to gravitational interactions-- drawn from the value of $\beta_{\lambda}$ is not physically meaningful.

[3]
Title: Singular vector structure of quantum curves
Comments: 33 pages; proceedings of the 2016 AMS von Neumann Symposium
Subjects: High Energy Physics - Theory (hep-th); Mathematical Physics (math-ph); Quantum Algebra (math.QA)

We show that quantum curves arise in infinite families and have the structure of singular vectors of a relevant symmetry algebra. We analyze in detail the case of the hermitian one-matrix model with the underlying Virasoro algebra, and the super-eigenvalue model with the underlying super-Virasoro algebra. In the Virasoro case we relate singular vector structure of quantum curves to the topological recursion, and in the super-Virasoro case we introduce the notion of super-quantum curves. We also discuss the double quantum structure of the quantum curves and analyze specific examples of Gaussian and multi-Penner models.

[4]
Title: Interaction of Non-Abelian Tensor Gauge Fields
Authors: George Savvidy
Subjects: High Energy Physics - Theory (hep-th)

The non-Abelian tensor gauge fields take value in extended Poincar\'e algebra. In order to define the invariant Lagrangian we introduce a vector variable in two alternative ways: through the transversal representation of the extended Poincar\'e algebra and through the path integral over the auxiliary vector field with the U(1) Abelian action. We demonstrate that this allows to fix the unitary gauge and derive scattering amplitudes in spinor representation.

[5]
Title: Ghost-free theory with third-order time derivatives
Subjects: High Energy Physics - Theory (hep-th); Cosmology and Nongalactic Astrophysics (astro-ph.CO); General Relativity and Quantum Cosmology (gr-qc)

As the first step to extend our understanding of higher-derivative theories, within the framework of analytic mechanics of interacting particles, we construct a ghost-free theory involving third-order time derivative in Lagrangian. We clarify that there is a crucial difference in construction from up-to-second-order-derivative theories. While eliminating linear momentum terms in the Hamiltonian is necessary and sufficient to kill the ghosts associated with the higher derivatives for the Lagrangian with up to second-order derivatives, this is necessary but not sufficient for the Lagrangian with higher than second-order derivatives. We demonstrate that even after eliminating the linear momentum terms ghosts are still lurking and they need to be removed appropriately to make Lagrangian free from the ghosts. We clarify a set of ghost-free conditions under which we show that the Hamiltonian is bounded, and that equations of motion are reducible into a second-order system.

[6]
Title: Notes on $\widetilde{\mathrm{SL}}(2,\mathbb{R})$ representations
Authors: Alexei Kitaev
Subjects: High Energy Physics - Theory (hep-th); Mathematical Physics (math-ph)

These notes describe representations of the universal cover of $\mathrm{SL}(2,\mathbb{R})$ with a view toward applications in physics. Spinors on the hyperbolic plane and the two-dimensional anti-de Sitter space are also discussed.

[7]
Title: Gravitational collapse and Hawking-like radiation of the shell in AdS spacetime
Subjects: High Energy Physics - Theory (hep-th)

In this paper, we study the collapse of a massive shell in 2+1 and 3+1 dimensional gravity with Anti-de Sitter asymptotics. Using the Gauss-Codazzi method, we derive gravitational equations of motion of the shell. We then use the functional Schrodinger formalism to calculate the spectrum of particles produced during the collapse. At the late time, radiation agrees very well with the standard Hawking results. In 3+1 dimensions, we reproduce the Hawking-Page transition. We then construct the density matrix of this collapsing system and analyze the information content in the emitted radiation. We find that the off-diagonal elements of the density matrix are very important in preserving the unitarity of the system.

[8]
Title: Infinite (continuous) spin fields in the frame-like formalism
Subjects: High Energy Physics - Theory (hep-th)

In this paper we elaborate on the gauge invariant frame-like Lagrangian description for the wide class of the so-called infinite (or continuous) spin representations of Poincar\'e group. We use our previous results on the gauge invariant formalism for the massive mixed symmetry fields corresponding to the Young tableau with two rows Y(k,l) (Y(k+1/2,l+1/2) for the fermionic case). We have shown that the corresponding infinite spin solutions can be constructed as a limit where k goes to infinity, while l remain to be fixed and label different representations. Moreover, our gauge invariant formalism provides a natural generalization to (Anti) de Sitter spaces as well. As in the completely symmetric case considered earlier by Metsaev we have found that there are no unitary solutions in de Sitter space, while there exists a rather wide spectrum of Anti de Sitter ones. In this, the question what representations of the Anti de Sitter group such solutions correspond to remains to be open.

[9]
Title: AdS4 backgrounds with N>16 supersymmetries in 10 and 11 dimensions
Subjects: High Energy Physics - Theory (hep-th); Mathematical Physics (math-ph); Differential Geometry (math.DG)

We explore all warped $AdS_4\times_w M^{D-4}$ backgrounds with the most general allowed fluxes that preserve more than 16 supersymmetries in $D=10$- and $11$-dimensional supergravities. After imposing the assumption that either the internal space $M^{D-4}$ is compact without boundary or the isometry algebra of the background decomposes into that of AdS$_4$ and that of $M^{D-4}$, we find that there are no such backgrounds in IIB supergravity. Similarly in IIA supergravity, there is a unique such background with 24 supersymmetries locally isometric to $AdS_4\times \mathbb{CP}^3$, and in $D=11$ supergravity all such backgrounds are locally isometric to the maximally supersymmetric $AdS_4\times S^7$ solution.

[10]
Title: Weak gravitation from a small extra 2D sphere
Subjects: High Energy Physics - Theory (hep-th); General Relativity and Quantum Cosmology (gr-qc)

In order to explain weak gravitation in our 4-dimensional universe, a 6-dimensional model with a small extra 2D sphere is proposed. The traceless energy-momentum tensor is quite naturally appeared in our 6-dimensional model. The warp factor is given by $\phi (\theta ) = \epsilon + \sin{\theta }$, where $\epsilon$ plays a role of killing the singular point $\phi (\theta )=0$, and is assumed $0 < \epsilon \ll 1$. Any massive particle is rolling down into points along this geodesic line. The light ray can be shown to stay in our 4-dimensional universe. This suggest us that our 4-dimensional world can be located at $\theta =0$ and/or $\theta = \pi$, its background metric being $\epsilon ^2 \eta _{\mu \nu }$. As a result, we have the 4-dimensional Newton constant, which is given by $G_N \simeq G_6 \epsilon ^{10}$ and the fifth force coefficients appeared here are $\alpha _i\simeq \epsilon ^{2(i-4)}$, $i=1, 2, 3$. Here $G_6$ is the gravitational constant in 6-dimensional spacetime. If we take $\epsilon = 10^{-3.8}$ against $G_6\sim 1($GeV$)^{-2}$, we get $G_N\sim 10^{-38}($Gev$)^{-2}$, the present time gravitational constant.

[11]
Title: On the propagation of gravitational waves in a $Λ$CDM universe
Subjects: High Energy Physics - Theory (hep-th); General Relativity and Quantum Cosmology (gr-qc)

We study here how the presence of non-zero matter density and a cosmological constant could affect the observation of gravitational waves in Pulsar Timing Arrays. Conventionally, the effect of matter and cosmological constant is included by considering the redshift in frequency due to the expansion. However, there is an additional effect due to the change of coordinate systems from the natural ones in the region where waves are produced to the ones used to measure the pulsar timing residuals. This change is unavoidable as the strong gravitational field in a black hole merger distorts clocks and rules. Harmonic waves produced in such a merger become anharmonic when detected by a cosmological observer. The effect is small but appears to be observable for the type of gravitational waves to which PTA are sensitive and for the favoured values of the cosmological parameters.

[12]
Title: Near Horizon Geometry of Warped Black Holes in Generalized Minimal Massive Gravity
Comments: 15 pages, no figure. arXiv admin note: text overlap with arXiv:1701.00209, arXiv:1606.05260
Subjects: High Energy Physics - Theory (hep-th)

We consider spacelike warped AdS$_{3}$ black hole metric in Boyer-Lindquist coordinate system. We present a coordinates transformation so that it maps metric in Boyer-Lindquist coordinates to the one in Gaussian null coordinates. Then we introduce new fall-off conditions near the horizon of non-extremal warped black holes. We study the near horizon symmetry algebra of such solutions in the context of Generalized minimal massive gravity. Similar to the black flower solutions, also we obtain the Heisenberg algebra as the near horizon symmetry algebra of the warped black flower solutions. We show that the vacuum state and all descendants of the vacuum have the same energy. Thus these zero energy excitations on the horizon appear as soft hairs on the warped black hole.

[13]
Title: Fluctuations through a Vibrating Bounce
Subjects: High Energy Physics - Theory (hep-th); Cosmology and Nongalactic Astrophysics (astro-ph.CO); General Relativity and Quantum Cosmology (gr-qc)

We study the evolution of cosmological perturbations in a non-singular bouncing cosmology with a bounce phase which has superimposed oscillations of the scale factor. We identify length scales for which the final spectrum of fluctuations obtains imprints of the non-trivial bounce dynamics. These imprints in the spectrum are manifested in the form of damped oscillation features at scales smaller than a characteristic value and an increased reddening of the spectrum at all the scales as the number of small bounces increases.

[14]
Title: Spacetime from locality of interactions in deformations of special relativity: the example of $κ$-Poincaré Hopf algebra
Subjects: High Energy Physics - Theory (hep-th); General Relativity and Quantum Cosmology (gr-qc)

A new proposal for the notion of spacetime in a relativistic generalization of special relativity based on a modification of the composition law of momenta is presented. Locality of interactions is the principle which defines the spacetime structure for a system of particles. The formulation based on $\kappa$-Poincar\'e Hopf algebra is shown to be contained in this framework as a particular example.

[15]
Title: Holographic quenches and anomalous transport
Comments: Based on my master thesis, extended version of arXiv:1607.06817
Subjects: High Energy Physics - Theory (hep-th)

In my master thesis, I investigated the chiral-magnetic effect in the context of holography; I focused in especially on the impact of the chiral anomaly at transport properties and non-equilbrium behaviour in response to an holographic quench. Concretely, I considered an $U(1)_\text{A}\times U(1)_\text{V}$-Einstein-Maxwell bottom-up model consisting of two massless gauge fields, coupled by a Chern-Simons term in the fivedimensional AdS spacetime. The two gauge fields provide a time dependent electric field and a static magnetic field, parallel to it. As response of the system to quench, I investigated the electromagnetic current in direction of the magnetic field which is generated due to the CME. In the first part of the thesis, I characterised the initial response of the system, in a fixed Schwarzschild AdS background, subjected to a 'fast' quench. The corresponding hyperbolic PDE is solved by means of a fully spectral code in spaces as well as in time direction. Note that this was the first application of a fully spectral code within holography. In the case of 'fast' quenches, the system exhibits an universal scaling behaviour, independent of the external parameters as the strength of the anomaly and the magnetic field, respectively. The late time behaviour of the system shows, depending on the quench and external parameters, in some cases long lived oscillations in the current. Furthermore, I computed the quasi-normal modes of the systems, including the backreaction of the matter fields on the background metric. It turns out that the long lived oscillations appear only in presence of the anomaly and can be traced back to the presence of Landau levels in the system. The results of my master thesis were partly published in arXiv:1607.06817; however, the thesis contains a lot of interesting, and so far unpublished, results and can be viewed as extended version of the paper.

[16]
Title: Tree-level gluon amplitudes on the celestial sphere
Subjects: High Energy Physics - Theory (hep-th)

Pasterski, Shao and Strominger have recently proposed that massless scattering amplitudes can be mapped to correlators on the celestial sphere at infinity via a Mellin transform. We apply this prescription to arbitrary $n$-point tree-level gluon amplitudes. The Mellin transforms of MHV amplitudes are given by generalized hypergeometric functions on the Grassmannian $Gr(4,n)$, while generic non-MHV amplitudes are given by more complicated Gelfand $A$-hypergeometric functions.

[17]
Title: The Sudakov form factor at four loops in maximal super Yang-Mills theory
Subjects: High Energy Physics - Theory (hep-th); High Energy Physics - Phenomenology (hep-ph)

The four-loop Sudakov form factor in maximal super Yang-Mills theory is analysed in detail. It is shown explicitly how to construct a basis of integrals that have a uniformly transcendental expansion in the dimensional regularisation parameter, further elucidating the number-theoretic properties of Feynman integrals. The physical form factor is expressed in this basis for arbitrary colour factor. In the nonplanar sector the required integrals are integrated numerically using a mix of sector-decomposition and Mellin-Barnes representation methods. Both the cusp as well as the collinear anomalous dimension are computed. The results show explicitly the violation of quadratic Casimir scaling at the four-loop order. A thorough analysis concerning the reliability of reported numerical uncertainties is carried out.

[18]
Title: Magnetoydroynamics with chiral anomaly: phases of collective excitations and instabilities
Subjects: High Energy Physics - Theory (hep-th); Mesoscale and Nanoscale Physics (cond-mat.mes-hall); High Energy Physics - Phenomenology (hep-ph); Nuclear Theory (nucl-th)

We study the relativistic hydrodynamics with chiral anomaly and dynamical electromagnetic fields, Chiral MagnetoHydroDynamics (CMHD). We formulate the CMHD as a low-energy effective theory based on a derivative expansion. We demonstrate the modification of ordinary MagnetoHydroDynamics (MHD) due to chiral anomaly can be obtained from the second law of thermodynamics and is tied to chiral magnetic effect with the universal coefficient. When axial charge imbalance becomes larger than a critical value, a new type of collective gapless excitation in the CMHD appears, as a result of the interplay among magnetic field, flow velocity, and chiral anomaly; we call it "Chiral MagnetoHelical Mode" (CMHM). These modes carry definite magnetic and fluid helicities and will either grow exponentially or dissipate in time, depending on the relative sign between their helicity and axial charge density. The presence of exponentially growing CMHM indicates a hydrodynamic instability.

### Cross-lists for Thu, 23 Nov 17

[19]  arXiv:1711.08100 (cross-list from gr-qc) [pdf, other]
Title: Hairy AdS black holes with a toroidal horizon in 4D Einstein-nonlinear $σ$-model system
Comments: 15 pages, 1 figure. Accepted for publication in Physics Letters B
Subjects: General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Theory (hep-th)

An exact hairy asymptotically locally AdS black hole solution with a flat horizon in the Einstein-nonlinear sigma model system in (3+1) dimensions is constructed. The ansatz for the nonlinear $SU(2)$ field is regular everywhere and depends explicitly on Killing coordinates, but in such a way that its energy-momentum tensor is compatible with a metric with Killing fields. The solution is characterized by a discrete parameter which has neither topological nor Noether charge associated with it and therefore represents a hair. A $U(1)$ gauge field interacting with Einstein gravity can also be included. The thermodynamics is analyzed. Interestingly, the hairy black hole is always thermodynamically favored with respect to the corresponding black hole with vanishing Pionic field.

[20]  arXiv:1711.08270 (cross-list from hep-ph) [pdf, other]
Title: Natural cliff inflation
Subjects: High Energy Physics - Phenomenology (hep-ph); Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Physics - Theory (hep-th)

We propose a novel scenario of inflation, in which the inflaton is identified as the lightest mode of an angular field in a compactified fifth dimension. The periodic effective potential exhibits exponentially flat plateaus, so that a sub-Planckian field excursion without hilltop initial conditions is naturally realized. We can obtain consistent predictions with observations on the spectral index and the tensor-to-scalar ratio.

[21]  arXiv:1711.08292 (cross-list from gr-qc) [pdf, other]
Title: New black holes in $D=5$ minimal gauged supergravity: deformed boundaries and 'frozen' horizons
Subjects: General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Theory (hep-th)

A new class of black hole solutions of the five dimensional minimal gauged supergravity is presented. They are characterized by the mass, the electric charge, two equal magnitude angular momenta and the magnitude of the magnetic potential at infinity. These black holes possess a horizon of spherical topology; however, both the horizon and the sphere at infinity can be arbitrarily squashed, with nonextremal solutions interpolating between black strings and black branes. A particular set of extremal configurations corresponds to a new one-parameter family of supersymmetric black holes. While their conserved charges are determined by the squashing of the sphere at infinity, these supersymmetric solutions possess the same horizon geometry.

[22]  arXiv:1711.08354 (cross-list from hep-ph) [pdf, other]
Title: Pion Condensation by Rotation in a Magnetic field
Comments: 5 pages, 2 figures. arXiv admin note: text overlap with arXiv:1710.02895
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)

We show that the combined effects of a rotation plus a magnetic field can cause charged pion condensation. We suggest that this phenomenon may yield to observable effects in current heavy ion collisions at collider energies, where large magnetism and rotations are expected in off-central collisions.

[23]  arXiv:1711.08372 (cross-list from gr-qc) [pdf, ps, other]
Title: Black branes and black strings in the astrophysical and cosmological context
Comments: 7 pages, no figures and tables
Subjects: General Relativity and Quantum Cosmology (gr-qc); Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Physics - Theory (hep-th)

We consider Kaluza-Klein models where internal spaces are compact flat or curved Einstein spaces. This background is perturbed by a compact gravitating body with the dust-like equation of state (EoS) in the external/our space and an arbitrary EoS parameter $\Omega$ in the internal space. Without imposing any restrictions on the form of the perturbed metric and the distribution of the perturbed energy densities, we perform the general analysis of the Einstein and conservation equations in the weak-field limit. All conclusions follow from this analysis. For example, we demonstrate that the perturbed model is static and perturbed metric preserves the block-diagonal form. In a particular case $\Omega=-1/2$, the found solution corresponds to the weak-field limit of the black strings/branes. The black strings/branes are compact gravitating objects which have the topology (four-dimensional Schwarzschild spacetime)$\times$ ($d$-dimensional internal space) with $d\geq 1$. We present the arguments in favour of these objects. First, they satisfy the gravitational tests for the parameterized post-Newtonian parameter $\gamma$ at the same level of accuracy as General Relativity. Second, they are preferable from the thermodynamical point of view. Third, averaging over the Universe, they do not destroy the stabilization of the internal space. These are the astrophysical and cosmological aspects of the black strings/branes.

[24]  arXiv:1711.08415 (cross-list from math-ph) [pdf, ps, other]
Title: Holomorphic solutions of the susy $σ$-model and gauge invariance
Subjects: Mathematical Physics (math-ph); High Energy Physics - Theory (hep-th)

For the first time we develop the gauge invariance of the supersymmetric grassmannian sigma model $G(M,N)$. It is richer then its purely bosonic submodel and we show how to use it in order to reduce some constant curvature holomorphic solutions of the model into simpler expressions.

### Replacements for Thu, 23 Nov 17

[25]  arXiv:1510.06655 (replaced) [pdf, ps, other]
Title: On the Global Casimir Effect in the Schwarzschild Spacetime
Comments: New version with 15 pages and 3 figures. To appear in JCAP
Subjects: General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Theory (hep-th)
[26]  arXiv:1612.00700 (replaced) [pdf, ps, other]
Title: Radiative corrections and instability of large Q-Balls
Comments: 17 pages, 10 figures, referneces added, minor changes in the text
Journal-ref: Mod. Phys. Lett. A, Vol. 32, No. 37 (2017) 1750198
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)
[27]  arXiv:1705.03897 (replaced) [pdf, other]
Title: Surprises from Complete Vector Portal Theories: New Insights into the Dark Sector and its Interplay with Higgs Physics
Comments: 5 pages, 3 figures; v2: minor corrections, references added, journal version
Journal-ref: Phys.Rev. D96 (2017) no.9, 095006
Subjects: High Energy Physics - Phenomenology (hep-ph); Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Physics - Experiment (hep-ex); High Energy Physics - Theory (hep-th)
[28]  arXiv:1706.05669 (replaced) [pdf, ps, other]
Title: Diffusion constant of slowly rotating black three-brane
Journal-ref: Phys. Lett. B 776,58-63(2018)
Subjects: High Energy Physics - Theory (hep-th)
[29]  arXiv:1706.07011 (replaced) [pdf, other]
Title: Frame Covariant Nonminimal Multifield Inflation
Comments: 43 pages, 12 figures; typos corrected; references added; revised version resubmitted to journal
Subjects: High Energy Physics - Phenomenology (hep-ph); General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Theory (hep-th)
[30]  arXiv:1707.09452 (replaced) [pdf, other]
Title: Numerical solution of open string field theory in Schnabl gauge
Comments: 37 pages, 9 figures, some typos corrected
Subjects: High Energy Physics - Theory (hep-th)
[31]  arXiv:1708.03554 (replaced) [pdf, ps, other]
Title: Massive gravitons in arbitrary spacetimes
Comments: 7 pages, presentation is more detailed, Appendix expanded, eq.(12) corrected, references added
Subjects: High Energy Physics - Theory (hep-th); General Relativity and Quantum Cosmology (gr-qc)
[32]  arXiv:1708.04619 (replaced) [pdf, other]
Title: Quantum Field Theory of X-Cube Fracton Topological Order and Robust Degeneracy from Geometry
Comments: 14+6 pages, 8+3 figures; v3 fixes some minor mistakes
Journal-ref: Phys. Rev. B 96, 195139 (2017)
Subjects: Strongly Correlated Electrons (cond-mat.str-el); High Energy Physics - Theory (hep-th)
[33]  arXiv:1710.04811 (replaced) [pdf, other]
Title: Electroweak Symmetry Breaking and Mass Spectra in Six-Dimensional Gauge-Higgs Grand Unification
Comments: 58 pages, 7 tables, 2 figures
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)
[34]  arXiv:1710.04816 (replaced) [pdf, other]
Title: Non-perturbative to perturbative QCD via the FFBRST
Comments: 10 Pages, Enlarged and revised substantially with new insights
Subjects: High Energy Physics - Theory (hep-th)
[35]  arXiv:1710.07252 (replaced) [pdf, other]
Title: Conserved Charges in Extended Theories of Gravity
Subjects: High Energy Physics - Theory (hep-th); General Relativity and Quantum Cosmology (gr-qc)
[36]  arXiv:1710.08453 (replaced) [pdf, other]
Title: Singular geometry and Higgs bundles in string theory
Subjects: Differential Geometry (math.DG); High Energy Physics - Theory (hep-th); Algebraic Geometry (math.AG)
[37]  arXiv:1711.01737 (replaced) [pdf, ps, other]
Title: Quantum monopole via Heisenberg quantization
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)
[38]  arXiv:1711.02063 (replaced) [pdf, other]
Title: Cluster integrable systems, q-Painleve equations and their quantization
Subjects: Mathematical Physics (math-ph); High Energy Physics - Theory (hep-th); Exactly Solvable and Integrable Systems (nlin.SI)
[39]  arXiv:1711.02259 (replaced) [pdf, other]
Title: Information Transfer and Coarse-Graining in Eternal Black Holes
Authors: Dongsu Bak
Comments: 13 pages, 5 figures, typos corrected and slight refinement
Subjects: High Energy Physics - Theory (hep-th)
[40]  arXiv:1711.02330 (replaced) [pdf, other]
Title: A bare quantum null energy condition
Comments: 4 pages, no figure; v2: minor corrections
Subjects: High Energy Physics - Theory (hep-th); General Relativity and Quantum Cosmology (gr-qc)
[41]  arXiv:1711.03737 (replaced) [pdf, ps, other]
Title: Soft Theorems For Shift-Symmetric Cosmologies