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Related papers: String stars in $d\geq 7$

200 papers

We discuss heterotic string theories in two dimensions with gauge groups Spin(24) and Spin(8) x E_8. After compactification the theories exhibit a rich spectrum of states with both winding and momentum. At special points some of these…

High Energy Physics - Theory · Physics 2009-11-11 Joshua L. Davis , Finn Larsen , Nathan Seiberg

The quest for extension of holographic correspondence to the case of finite temperature naturally includes Kerr-AdS black holes and their field theory duals. We probe the five-dimensional Kerr-AdS space time by pulsating strings. First we…

High Energy Physics - Theory · Physics 2022-05-05 O. V. Geytota , A. A. Golubtsova , H. Dimov , Vu H. Nguyen , R. C. Rashkov

We consider the thermodynamics of a color-confined phase of quantum chromodynamics (QCD) and pure gauge theory within a string-inspired model, corresponding to a physical spatial dimension, d = 3. We show that the physical mass spectrum of…

High Energy Physics - Phenomenology · Physics 2025-11-10 Michał Marczenko , Győző Kovács , Larry McLerran , Krzysztof Redlich

We investigate the evolution of small perturbations around black strings and branes which are low energy solutions of string theory. For simplicity we focus attention on the zero charge case and show that there are unstable modes for a…

High Energy Physics - Theory · Physics 2009-01-23 R. Gregory , R. Laflamme

Utilising the master equation with source for perturbations of the Schwarzschild-Tangherlini solution, we construct perturbative solutions representing a black hole accelerated by a string in higher dimensions. We show that such solutions…

High Energy Physics - Theory · Physics 2009-01-25 Hideo Kodama

The dynamics of a probe particle or wrapped brane moving in the two-dimensional Rindler space can be described by a time-dependent tachyon field theory. Using knowledge of tachyon condensation, we learn that the infalling brane gets…

High Energy Physics - Theory · Physics 2015-06-03 Huiquan Li

We discuss semi-classical string configurations at finite temperature. We find that those soliton solution in the background describing type IIA strings disappear or become divergent when we approach the Hagedorn temperature in the strong…

High Energy Physics - Theory · Physics 2009-05-25 J. D. Madrigal , P. Talavera

We calculate the tidal Love numbers of black holes and neutron stars in the presence of higher dimensions. The perturbation equations around an arbitrary static and spherically symmetric metric for the even parity modes are presented in the…

General Relativity and Quantum Cosmology · Physics 2019-01-30 Kabir Chakravarti , Sumanta Chakraborty , Sukanta Bose , Soumitra SenGupta

We consider black hole production at the LHC in a generic scenario with many extra dimensions where the Standard Model fields are confined to a brane. With $\sim 20$ dimensions the hierarchy problem is shown to be naturally solved without…

High Energy Physics - Phenomenology · Physics 2009-11-11 JoAnne L. Hewett , Ben Lillie , Thomas G. Rizzo

In this work we derive non-singular BPS string solutions from an action that captures the essential features of a D-brane-anti-D-brane system compactified to four dimensions. The model we consider is a supersymmetric abelian Higgs model…

High Energy Physics - Theory · Physics 2009-11-11 Jose J. Blanco-Pillado , Gia Dvali , Michele Redi

The thermodynamics of a gas of strings and D-branes near the Hagedorn transition is described by a coupled set of Boltzmann equations for weakly interacting open and closed long strings. The resulting distributions are dominated by the open…

High Energy Physics - Theory · Physics 2008-11-26 Sangmin Lee , Larus Thorlacius

We study a d-dimensional FRW universe, containing a perfect fluid with p = w \rho and \frac{1} {d - 1} \le w \le 1, and find a correspondence principle similar to that of Horowitz and Polchinski in the black hole case. This principle…

High Energy Physics - Theory · Physics 2008-11-26 S. Kalyana Rama

According to string theory, string ball is a highly excited long string which decays to standard model particles at the Hagedorn temperature with thermal spectrum. If there are extra dimensions, the string scale can be $\sim$ TeV, and we…

High Energy Physics - Phenomenology · Physics 2009-07-22 Gouranga C Nayak

In this paper, we obtain two different static black string solutions by considering as sources axisymmetric dark matter distributions in 3+1 dimensions. These solutions tend asymptotically to the usual static and uncharged black string…

General Relativity and Quantum Cosmology · Physics 2023-05-17 Marcony S. Cunha , G. Alencar , Celio R. Muniz , Valdir B. Bezerra , Horácio S. Vieira

We study the thermodynamic properties of a static electrically charged spherical thin shell in $d$ dimensions by imposing the first law of thermodynamics on the shell. The shell is at radius $R$, inside it the spacetime is Minkowski, and…

General Relativity and Quantum Cosmology · Physics 2022-11-28 Tiago V. Fernandes , José P. S. Lemos

Recent progress on string theory in curved spacetimes is reviewed. The string dynamics in cosmological and black hole spacetimes is investigated.The methods to solve the string equations of motion in curved spacetimes are described.That is,…

High Energy Physics - Theory · Physics 2007-05-23 H. J. de Vega , N. sánchez

We construct spherically symmetric boson star solutions in $D \in \{4,5,6\}$ spacetime dimensions, considering the effects of both a quartic self-interaction term and a solitonic potential. We then perform a perturbative analysis,…

General Relativity and Quantum Cosmology · Physics 2025-10-17 Gareth Arturo Marks , Abdullah Al Zaif

Motivated by the desire to better understand finite-temperature holography for three-dimensional Schroedinger spacetimes, we: i) construct a four-parameter family of warped black string solutions of type IIB supergravity and ii) find the…

High Energy Physics - Theory · Physics 2015-06-12 Stephane Detournay , Monica Guica

In string theory, black holes have a minimum mass below which they transition into highly excited long and jagged strings --- ``string balls''. These are the stringy progenitors of black holes; because they are lighter, in theories of…

High Energy Physics - Phenomenology · Physics 2009-11-07 Savas Dimopoulos , Roberto Emparan

Drawing on insights from the Swampland program, we initiate a classification of infinite distance limits in the conformal manifolds of 4d SCFTs. Each limit is characterized by a Hagedorn-like behavior of the large $N$ density of states,…

High Energy Physics - Theory · Physics 2024-10-11 José Calderón-Infante , Irene Valenzuela