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We explicitly show that the net number of degrees of freedom in the two-dimensional dilaton gravity is zero through the Hamiltonian constraint analysis. This implies that the local space-time dependent physical excitations do not exist.…

High Energy Physics - Theory · Physics 2016-09-06 Won T. Kim , Julian Lee , Young Jai Park

We study the properties of two-dimensional dilatonic black holes from the viewpoint of geometrothermodynamics. We show that the thermodynamic curvature of the equilibrium space vanishes only in the case of a flat spacetime, and it…

General Relativity and Quantum Cosmology · Physics 2015-05-13 Hernando Quevedo , Alberto Sanchez

We describe a new scenario for the formation of primordial black holes (PBHs). In the early Universe, the long-range forces mediated by the scalar fields can lead to formation of halos of heavy particles even during the radiation-dominated…

Cosmology and Nongalactic Astrophysics · Physics 2021-01-28 Marcos M. Flores , Alexander Kusenko

We study black hole formation in a model of two dimensional dilaton gravity and 24 massless scalar fields with a boundary. We find the most general boundary condition consistent with perfect reflection of matter and the constraints. We show…

High Energy Physics - Theory · Physics 2010-11-01 Sumit R. Das , Sudipta Mukherji

Type-II Weyl fermions may emerge behind the event horizon of black holes. We employ the Painlev\'e-Gullstrand metric to study the surface of the Lifshitz transition at the horizon, equivalent to the interface separating the type-I and…

Mesoscale and Nanoscale Physics · Physics 2026-05-28 Iftekher S. Chowdhury , Hom Nath Dhungana , Shah Haque , Hind Adawi , Eric Howard

Black holes with masses below approximately $10^{15}$ g are expected to emit gamma rays with energies above a few tens of MeV, which can be detected by the Fermi Large Area Telescope (LAT). Although black holes with these masses cannot be…

High Energy Astrophysical Phenomena · Physics 2018-02-02 LAT Collaboration

The Dirac equation is solved in the Einstein-Yang-Mills background found by Bartnik and McKinnon. We find a normalizable zero-energy fermion mode in the $s$-wave sector. As shown recently, their solution corresponds to a gravitational…

General Relativity and Quantum Cosmology · Physics 2009-10-07 G. W. Gibbons , Alan R. Steif

This work deals with the formation of black hole in bidimensional dilaton gravity coupled to scalar matter fields. We investigate two scalar matter systems, one described by a sixth power potential and the other defined with two scalar…

High Energy Physics - Theory · Physics 2009-10-31 M. Alves , D. Bazeia , V. B. Bezerra

Driven by the landscape of garden-variety condensed matter systems, we have investigated how the dual spectral function behaves at the non-relativistic as well as relativistic fermionic fixed point by considering the probe Dirac fermion in…

High Energy Physics - Theory · Physics 2012-02-01 Wei-Jia Li , Rene Meyer , Hongbao Zhang

We study the conditions for 2-dimensional dilaton gravity models to have dynamical formation of black holes and construct all such models. Furthermore we present a parametric representation of the general solutions of the black holes.

General Relativity and Quantum Cosmology · Physics 2014-11-17 T. Futamase , M. Hotta , Y. Itoh

If the scale of quantum gravity is near a TeV, black holes will be copiously produced at the LHC. In this work we study the main properties of the light descendants of these black holes. We show that the emitted partons are closely spaced…

High Energy Physics - Phenomenology · Physics 2008-11-26 Luis Anchordoqui , Haim Goldberg

We are entering a new era to test the strong gravity regime around astrophysical black holes. The possibility that they are actually horizonless ultracompact objects and then free from the information loss paradox can be examined more…

General Relativity and Quantum Cosmology · Physics 2019-12-11 Jing Ren

If we consider the gravitational collapse of a material object to a black hole, we would expect, for ranges of mass where a black hole would form, the following scenario. A large enough object would collapse classically until an event…

General Relativity and Quantum Cosmology · Physics 2008-11-26 L. Ortíz , M. P. Ryan

We study fermionic perturbations in the background of a two and five-dimensional dilatonic black holes. Then, we compute the reflection and transmission coefficients and the absorption cross section for fermionic fields, and we show…

General Relativity and Quantum Cosmology · Physics 2015-06-19 Ramón Becar , P. A. González , Yerko Vásquez

For a large enough Schwarzschild black hole, the horizon is a region of space where gravitational forces are weak; yet it is also a region leading to numerous puzzles connected to stringy physics. In this work, we analyze the process of…

High Energy Physics - Theory · Physics 2008-11-26 Anand Murugan , Vatche Sahakian

We present a scenario for non-thermal production of dark matter from evaporation of primordial black holes. A period of very early matter domination leads to formation of black holes with a maximum mass of $\simeq 2 \times 10^8$ g, whose…

Cosmology and Nongalactic Astrophysics · Physics 2018-03-15 Rouzbeh Allahverdi , James B. Dent , Jacek Osinski

In this paper we investigate the problem of fermion creation inside a three dimensional box. We present an appropriate wave function which satisfies the Dirac equation in this geometry with MIT bag model boundary condition. We consider…

High Energy Physics - Theory · Physics 2015-06-04 M. R. Setare , A. Seyedzahedi

We consider gas of massless fermions at certain temperature T and acceleration a. We find a second order phase transition at temperature T approaching the Unruh temperature TU. The implications for hadronization of the quark-gluon plasma…

High Energy Physics - Theory · Physics 2024-10-07 Georgy Yu. Prokhorov , Oleg V. Teryaev , Valentin I. Zakharov

We study primordial black hole (PBH) formation in a minimally coupled $f(T)$ teleparallel cosmology that generates a transient departure from standard radiation domination. The model is constructed so that modified-gravity effects are…

General Relativity and Quantum Cosmology · Physics 2026-03-27 Gerasimos Kouniatalis , Theodoros Papanikolaou , Spyros Basilakos , Emmanuel N. Saridakis

Antisymmetric tensor field (two-form field) is a ubiquitous component in string theory and generally couples to the scalar sector through its kinetic term. In this paper, we propose a cosmological scenario that the particle production of…

Cosmology and Nongalactic Astrophysics · Physics 2023-10-26 Tomohiro Fujita , Hiromasa Nakatsuka , Ippei Obata , Sam Young