High Energy Physics  Theory
New submissions
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New submissions for Thu, 23 Nov 17
 [1] arXiv:1711.07990 [pdf, other]

Title: A matrix CFT at multiple large chargesAuthors: Orestis LoukasComments: 1+36 pages, 2 figuresSubjects: High Energy Physics  Theory (hepth)
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 largecharge 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] arXiv:1711.08009 [pdf, other]

Title: Unimodular Gravity and General Relativity UV divergent contributions to the scattering of massive scalar particlesComments: 13 pages, 4 figuresSubjects: High Energy Physics  Theory (hepth)
We work out the oneloop 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 nonvanishing 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] arXiv:1711.08031 [pdf, ps, other]

Title: Singular vector structure of quantum curvesComments: 33 pages; proceedings of the 2016 AMS von Neumann SymposiumSubjects: High Energy Physics  Theory (hepth); Mathematical Physics (mathph); 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 onematrix model with the underlying Virasoro algebra, and the supereigenvalue model with the underlying superVirasoro algebra. In the Virasoro case we relate singular vector structure of quantum curves to the topological recursion, and in the superVirasoro case we introduce the notion of superquantum curves. We also discuss the double quantum structure of the quantum curves and analyze specific examples of Gaussian and multiPenner models.
 [4] arXiv:1711.08034 [pdf, ps, other]

Title: Interaction of NonAbelian Tensor Gauge FieldsAuthors: George SavvidyComments: 13 pagesSubjects: High Energy Physics  Theory (hepth)
The nonAbelian 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] arXiv:1711.08125 [pdf, ps, other]

Title: Ghostfree theory with thirdorder time derivativesComments: 5 pagesSubjects: High Energy Physics  Theory (hepth); Cosmology and Nongalactic Astrophysics (astroph.CO); General Relativity and Quantum Cosmology (grqc)
As the first step to extend our understanding of higherderivative theories, within the framework of analytic mechanics of interacting particles, we construct a ghostfree theory involving thirdorder time derivative in Lagrangian. We clarify that there is a crucial difference in construction from uptosecondorderderivative 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 secondorder derivatives, this is necessary but not sufficient for the Lagrangian with higher than secondorder 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 ghostfree conditions under which we show that the Hamiltonian is bounded, and that equations of motion are reducible into a secondorder system.
 [6] arXiv:1711.08169 [pdf, other]

Title: Notes on $\widetilde{\mathrm{SL}}(2,\mathbb{R})$ representationsAuthors: Alexei KitaevComments: 27 pagesSubjects: High Energy Physics  Theory (hepth); Mathematical Physics (mathph)
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 twodimensional antide Sitter space are also discussed.
 [7] arXiv:1711.08182 [pdf, other]

Title: Gravitational collapse and Hawkinglike radiation of the shell in AdS spacetimeSubjects: High Energy Physics  Theory (hepth)
In this paper, we study the collapse of a massive shell in 2+1 and 3+1 dimensional gravity with Antide Sitter asymptotics. Using the GaussCodazzi 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 HawkingPage transition. We then construct the density matrix of this collapsing system and analyze the information content in the emitted radiation. We find that the offdiagonal elements of the density matrix are very important in preserving the unitarity of the system.
 [8] arXiv:1711.08223 [pdf, ps, other]

Title: Infinite (continuous) spin fields in the framelike formalismComments: 37 pages, 6 figuresSubjects: High Energy Physics  Theory (hepth)
In this paper we elaborate on the gauge invariant framelike Lagrangian description for the wide class of the socalled 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] arXiv:1711.08280 [pdf, ps, other]

Title: AdS4 backgrounds with N>16 supersymmetries in 10 and 11 dimensionsComments: 53 pagesSubjects: High Energy Physics  Theory (hepth); Mathematical Physics (mathph); Differential Geometry (math.DG)
We explore all warped $AdS_4\times_w M^{D4}$ 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 $M^{D4}$ is compact without boundary or the isometry algebra of the background decomposes into that of AdS$_4$ and that of $M^{D4}$, 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] arXiv:1711.08312 [pdf, ps, other]

Title: Weak gravitation from a small extra 2D sphereComments: 16 pages, no figuresSubjects: High Energy Physics  Theory (hepth); General Relativity and Quantum Cosmology (grqc)
In order to explain weak gravitation in our 4dimensional universe, a 6dimensional model with a small extra 2D sphere is proposed. The traceless energymomentum tensor is quite naturally appeared in our 6dimensional 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 4dimensional universe. This suggest us that our 4dimensional 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 4dimensional Newton constant, which is given by $G_N \simeq G_6 \epsilon ^{10}$ and the fifth force coefficients appeared here are $\alpha _i\simeq \epsilon ^{2(i4)}$, $i=1, 2, 3$. Here $G_6$ is the gravitational constant in 6dimensional 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] arXiv:1711.08315 [pdf, ps, other]

Title: On the propagation of gravitational waves in a $Λ$CDM universeComments: 18 pages, 2 figuresSubjects: High Energy Physics  Theory (hepth); General Relativity and Quantum Cosmology (grqc)
We study here how the presence of nonzero 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] arXiv:1711.08344 [pdf, ps, other]

Title: Near Horizon Geometry of Warped Black Holes in Generalized Minimal Massive GravityComments: 15 pages, no figure. arXiv admin note: text overlap with arXiv:1701.00209, arXiv:1606.05260Subjects: High Energy Physics  Theory (hepth)
We consider spacelike warped AdS$_{3}$ black hole metric in BoyerLindquist coordinate system. We present a coordinates transformation so that it maps metric in BoyerLindquist coordinates to the one in Gaussian null coordinates. Then we introduce new falloff conditions near the horizon of nonextremal 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] arXiv:1711.08370 [pdf, other]

Title: Fluctuations through a Vibrating BounceComments: 17 pages, 5 figuresSubjects: High Energy Physics  Theory (hepth); Cosmology and Nongalactic Astrophysics (astroph.CO); General Relativity and Quantum Cosmology (grqc)
We study the evolution of cosmological perturbations in a nonsingular 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 nontrivial 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] arXiv:1711.08403 [pdf, ps, other]

Title: Spacetime from locality of interactions in deformations of special relativity: the example of $κ$Poincaré Hopf algebraComments: 14 pagesSubjects: High Energy Physics  Theory (hepth); General Relativity and Quantum Cosmology (grqc)
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] arXiv:1711.08422 [pdf, other]

Title: Holographic quenches and anomalous transportAuthors: Sebastian GrieningerComments: Based on my master thesis, extended version of arXiv:1607.06817Subjects: High Energy Physics  Theory (hepth)
In my master thesis, I investigated the chiralmagnetic effect in the context of holography; I focused in especially on the impact of the chiral anomaly at transport properties and nonequilbrium behaviour in response to an holographic quench. Concretely, I considered an $U(1)_\text{A}\times U(1)_\text{V}$EinsteinMaxwell bottomup model consisting of two massless gauge fields, coupled by a ChernSimons 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 quasinormal 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] arXiv:1711.08435 [pdf, other]

Title: Treelevel gluon amplitudes on the celestial sphereComments: 13 pagesSubjects: High Energy Physics  Theory (hepth)
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 treelevel gluon amplitudes. The Mellin transforms of MHV amplitudes are given by generalized hypergeometric functions on the Grassmannian $Gr(4,n)$, while generic nonMHV amplitudes are given by more complicated Gelfand $A$hypergeometric functions.
 [17] arXiv:1711.08449 [pdf, ps, other]

Title: The Sudakov form factor at four loops in maximal super YangMills theoryComments: 47 pages, 17 figuresSubjects: High Energy Physics  Theory (hepth); High Energy Physics  Phenomenology (hepph)
The fourloop Sudakov form factor in maximal super YangMills 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 numbertheoretic 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 sectordecomposition and MellinBarnes 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 fourloop order. A thorough analysis concerning the reliability of reported numerical uncertainties is carried out.
 [18] arXiv:1711.08450 [pdf, other]

Title: Magnetoydroynamics with chiral anomaly: phases of collective excitations and instabilitiesComments: 8 pages, 3 figuresSubjects: High Energy Physics  Theory (hepth); Mesoscale and Nanoscale Physics (condmat.meshall); High Energy Physics  Phenomenology (hepph); Nuclear Theory (nuclth)
We study the relativistic hydrodynamics with chiral anomaly and dynamical electromagnetic fields, Chiral MagnetoHydroDynamics (CMHD). We formulate the CMHD as a lowenergy 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.
Crosslists for Thu, 23 Nov 17
 [19] arXiv:1711.08100 (crosslist from grqc) [pdf, other]

Title: Hairy AdS black holes with a toroidal horizon in 4D Einsteinnonlinear $σ$model systemComments: 15 pages, 1 figure. Accepted for publication in Physics Letters BSubjects: General Relativity and Quantum Cosmology (grqc); High Energy Physics  Theory (hepth)
An exact hairy asymptotically locally AdS black hole solution with a flat horizon in the Einsteinnonlinear 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 energymomentum 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 (crosslist from hepph) [pdf, other]

Title: Natural cliff inflationComments: 5 pages, 2 figuresSubjects: High Energy Physics  Phenomenology (hepph); Cosmology and Nongalactic Astrophysics (astroph.CO); High Energy Physics  Theory (hepth)
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 subPlanckian field excursion without hilltop initial conditions is naturally realized. We can obtain consistent predictions with observations on the spectral index and the tensortoscalar ratio.
 [21] arXiv:1711.08292 (crosslist from grqc) [pdf, other]

Title: New black holes in $D=5$ minimal gauged supergravity: deformed boundaries and 'frozen' horizonsComments: 5 pages, 4 figuresSubjects: General Relativity and Quantum Cosmology (grqc); High Energy Physics  Theory (hepth)
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 oneparameter 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 (crosslist from hepph) [pdf, other]

Title: Pion Condensation by Rotation in a Magnetic fieldComments: 5 pages, 2 figures. arXiv admin note: text overlap with arXiv:1710.02895Subjects: High Energy Physics  Phenomenology (hepph); High Energy Physics  Theory (hepth); Nuclear Experiment (nuclex); Nuclear Theory (nuclth)
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 offcentral collisions.
 [23] arXiv:1711.08372 (crosslist from grqc) [pdf, ps, other]

Title: Black branes and black strings in the astrophysical and cosmological contextComments: 7 pages, no figures and tablesSubjects: General Relativity and Quantum Cosmology (grqc); Cosmology and Nongalactic Astrophysics (astroph.CO); High Energy Physics  Theory (hepth)
We consider KaluzaKlein models where internal spaces are compact flat or curved Einstein spaces. This background is perturbed by a compact gravitating body with the dustlike 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 weakfield limit. All conclusions follow from this analysis. For example, we demonstrate that the perturbed model is static and perturbed metric preserves the blockdiagonal form. In a particular case $\Omega=1/2$, the found solution corresponds to the weakfield limit of the black strings/branes. The black strings/branes are compact gravitating objects which have the topology (fourdimensional 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 postNewtonian 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 (crosslist from mathph) [pdf, ps, other]

Title: Holomorphic solutions of the susy $σ$model and gauge invarianceComments: 8 pages, no figuresSubjects: Mathematical Physics (mathph); High Energy Physics  Theory (hepth)
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 SpacetimeComments: New version with 15 pages and 3 figures. To appear in JCAPSubjects: General Relativity and Quantum Cosmology (grqc); High Energy Physics  Theory (hepth)
 [26] arXiv:1612.00700 (replaced) [pdf, ps, other]

Title: Radiative corrections and instability of large QBallsComments: 17 pages, 10 figures, referneces added, minor changes in the textJournalref: Mod. Phys. Lett. A, Vol. 32, No. 37 (2017) 1750198Subjects: High Energy Physics  Phenomenology (hepph); High Energy Physics  Theory (hepth)
 [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 PhysicsComments: 5 pages, 3 figures; v2: minor corrections, references added, journal versionJournalref: Phys.Rev. D96 (2017) no.9, 095006Subjects: High Energy Physics  Phenomenology (hepph); Cosmology and Nongalactic Astrophysics (astroph.CO); High Energy Physics  Experiment (hepex); High Energy Physics  Theory (hepth)
 [28] arXiv:1706.05669 (replaced) [pdf, ps, other]

Title: Diffusion constant of slowly rotating black threebraneJournalref: Phys. Lett. B 776,5863(2018)Subjects: High Energy Physics  Theory (hepth)
 [29] arXiv:1706.07011 (replaced) [pdf, other]

Title: Frame Covariant Nonminimal Multifield InflationComments: 43 pages, 12 figures; typos corrected; references added; revised version resubmitted to journalSubjects: High Energy Physics  Phenomenology (hepph); General Relativity and Quantum Cosmology (grqc); High Energy Physics  Theory (hepth)
 [30] arXiv:1707.09452 (replaced) [pdf, other]

Title: Numerical solution of open string field theory in Schnabl gaugeComments: 37 pages, 9 figures, some typos correctedSubjects: High Energy Physics  Theory (hepth)
 [31] arXiv:1708.03554 (replaced) [pdf, ps, other]

Title: Massive gravitons in arbitrary spacetimesComments: 7 pages, presentation is more detailed, Appendix expanded, eq.(12) corrected, references addedSubjects: High Energy Physics  Theory (hepth); General Relativity and Quantum Cosmology (grqc)
 [32] arXiv:1708.04619 (replaced) [pdf, other]

Title: Quantum Field Theory of XCube Fracton Topological Order and Robust Degeneracy from GeometryComments: 14+6 pages, 8+3 figures; v3 fixes some minor mistakesJournalref: Phys. Rev. B 96, 195139 (2017)Subjects: Strongly Correlated Electrons (condmat.strel); High Energy Physics  Theory (hepth)
 [33] arXiv:1710.04811 (replaced) [pdf, other]

Title: Electroweak Symmetry Breaking and Mass Spectra in SixDimensional GaugeHiggs Grand UnificationComments: 58 pages, 7 tables, 2 figuresSubjects: High Energy Physics  Phenomenology (hepph); High Energy Physics  Theory (hepth)
 [34] arXiv:1710.04816 (replaced) [pdf, other]

Title: Nonperturbative to perturbative QCD via the FFBRSTComments: 10 Pages, Enlarged and revised substantially with new insightsSubjects: High Energy Physics  Theory (hepth)
 [35] arXiv:1710.07252 (replaced) [pdf, other]

Title: Conserved Charges in Extended Theories of GravityComments: 114 pages, 1 figure, a review, references addedSubjects: High Energy Physics  Theory (hepth); General Relativity and Quantum Cosmology (grqc)
 [36] arXiv:1710.08453 (replaced) [pdf, other]

Title: Singular geometry and Higgs bundles in string theoryComments: 24 pages. v2 details added to Open Question 1Subjects: Differential Geometry (math.DG); High Energy Physics  Theory (hepth); Algebraic Geometry (math.AG)
 [37] arXiv:1711.01737 (replaced) [pdf, ps, other]

Title: Quantum monopole via Heisenberg quantizationAuthors: Vladimir DzhunushalievComments: 8 pages, 5 figuresSubjects: High Energy Physics  Phenomenology (hepph); High Energy Physics  Theory (hepth)
 [38] arXiv:1711.02063 (replaced) [pdf, other]

Title: Cluster integrable systems, qPainleve equations and their quantizationComments: 28 pages v.2; 30 pages references added, misprints correctedSubjects: Mathematical Physics (mathph); High Energy Physics  Theory (hepth); Exactly Solvable and Integrable Systems (nlin.SI)
 [39] arXiv:1711.02259 (replaced) [pdf, other]

Title: Information Transfer and CoarseGraining in Eternal Black HolesAuthors: Dongsu BakComments: 13 pages, 5 figures, typos corrected and slight refinementSubjects: High Energy Physics  Theory (hepth)
 [40] arXiv:1711.02330 (replaced) [pdf, other]

Title: A bare quantum null energy conditionComments: 4 pages, no figure; v2: minor correctionsSubjects: High Energy Physics  Theory (hepth); General Relativity and Quantum Cosmology (grqc)
 [41] arXiv:1711.03737 (replaced) [pdf, ps, other]

Title: Soft Theorems For ShiftSymmetric CosmologiesComments: 4 pages; citation added in v2Subjects: High Energy Physics  Theory (hepth); Cosmology and Nongalactic Astrophysics (astroph.CO); General Relativity and Quantum Cosmology (grqc)
 [42] arXiv:1711.06776 (replaced) [pdf, ps, other]

Title: Generalized surface tension bounds in vacuum decayComments: 16 pagesSubjects: High Energy Physics  Theory (hepth)
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