Fate of Yang-Mills black hole in early Universe

AbstractDetecting the seed black holes from which quasars formed is extremely challenging; however, those seeds that did not grow into supermassive should be found as intermediate-mass black holes (IMBHs) of 100 – 105 M⊙ in local dwarf galaxies. The use of deep multiwavelength surveys has revealed that a population of actively accreting IMBHs (low-mass AGN) exists in dwarf galaxies at least out to z ˜3. The black hole occupation fraction of these galaxies suggests that the early Universe seed black holes formed from direct collapse of gas, which is reinforced by the possible flattening of the black hole-galaxy scaling relations at the low-mass end. This scenario is however challenged by the finding that AGN feedback can have a strong impact on dwarf galaxies, which implies that low-mass AGN in dwarf galaxies might not be the untouched relics of the early seed black holes. This has important implications for seed black hole formation models.

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$$P$$ P – $$V$$ V criticality of AdS black hole in the Einstein–Maxwell–power-Yang–Mills gravity

General Relativity and Gravitation ◽

10.1007/s10714-015-1851-2 ◽

2015 ◽

Vol 47 (2) ◽

Cited By ~ 18

Author(s):

Ming Zhang ◽

Zhan-Ying Yang ◽

De-Cheng Zou ◽

Wei Xu ◽

Rui-Hong Yue

Keyword(s):

Black Hole ◽

Yang Mills

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Analytic critical points of charged Rényi entropies from hyperbolic black holes

Journal of High Energy Physics ◽

10.1007/jhep05(2021)080 ◽

2021 ◽

Vol 2021 (5) ◽

Author(s):

Jie Ren

Keyword(s):

Black Holes ◽

Black Hole ◽

Study Phase ◽

Zero Temperature ◽

Charged Scalar ◽

Yang Mills ◽

Gravitational Systems ◽

Rényi Entropies ◽

Zero Entropy ◽

Renyi Entropies

Abstract We analytically study phase transitions of holographic charged Rényi entropies in two gravitational systems dual to the $$ \mathcal{N} $$ N = 4 super-Yang-Mills theory at finite density and zero temperature. The first system is the Reissner-Nordström-AdS5 black hole, which has finite entropy at zero temperature. The second system is a charged dilatonic black hole in AdS5, which has zero entropy at zero temperature. Hyperbolic black holes are employed to calculate the Rényi entropies with the entangling surface being a sphere. We perturb each system by a charged scalar field, and look for a zero mode signaling the instability of the extremal hyperbolic black hole. Zero modes as well as the leading order of the full retarded Green’s function are analytically solved for both systems, in contrast to previous studies in which only the IR (near horizon) instability was analytically treated.

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THERMODYNAMICS OF CONSTANT CURVATURE BLACK HOLES THROUGH SEMICLASSICAL TUNNELING

Modern Physics Letters A ◽

10.1142/s0217732311035444 ◽

2011 ◽

Vol 26 (13) ◽

pp. 937-947 ◽

Cited By ~ 3

Author(s):

ALEXANDRE YALE

Keyword(s):

Black Holes ◽

Black Hole ◽

Constant Curvature ◽

Hawking Radiation ◽

Emission Rate ◽

Yang Mills ◽

Fermion Fields ◽

Tunneling Method ◽

Semiclassical Tunneling ◽

Algorithmic Procedure

We study the semiclassical tunneling of scalar and fermion fields from the horizon of a Constant Curvature Black Hole, which is locally AdS and whose five-dimensional analogue is dual to [Formula: see text] super-Yang–Mills. In particular, we highlight the strong reliance of the tunneling method for Hawking radiation on near-horizon symmetries, a fact often hidden behind the algorithmic procedure with which the tunneling approach tends to be used. We ultimately calculate the emission rate of scalars and fermions, and hence the black hole's Hawking temperature.

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Using Lorentz Violation for Early Universe GW Generation Due to Black Hole Destruction in the Early Universe as by Freeze

10.20944/preprints202104.0657.v1 ◽

2021 ◽

Author(s):

Andrew W Beckwith

Keyword(s):

Black Holes ◽

Black Hole ◽

Dark Energy ◽

Early Universe ◽

Physical Mechanism ◽

Lorentz Violation ◽

Graviton Mass ◽

Work Done ◽

Momentum Relation

We are using information from a paper deriving a Lorentz-violating energy-momentum relation entailing an exact mo_mentum cutof as stated by G. Salesi . Salesi in his work allegedly defines Pre Planckian physics, whereas we restrict our given application to GW generation and DE formation in the first 10^-39s to 10^-33s or so seconds in the early universe. This procedure is inacted due to an earlier work whereas referees exhibited puzzlement as to the physical mechanism for release of Gravitons in the very early universe. The calculation is meant to be complementary to work done in the Book “Dark Energy” by M. Li, X-D. Li, and Y. Wang, and also a calculation for Black hole destruction as outlined by Karen Freeze, et. al. The GW generation will be when there is sufficient early universe density so as to break apart Relic Black holes but we claim that this destruction is directly linked to a Lorentz violating energy-momentum G. Salesi derived, which we adopt, with a mass m added in the G. Salesi energy momentum results proportional to a tiny graviton mass, times the number of gravitons in the first 10^-43 seconds

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Thermal relativity, corrections to black hole entropy, Born’s reciprocal relativity theory, and quantum gravity

Canadian Journal of Physics ◽

10.1139/cjp-2019-0034 ◽

2019 ◽

Vol 97 (12) ◽

pp. 1309-1316 ◽

Cited By ~ 2

Author(s):

Carlos Castro Perelman

Keyword(s):

Black Hole ◽

Quantum Gravity ◽

Black Hole Entropy ◽

Relativity Theory ◽

Yang Mills ◽

Newman Black Hole ◽

Maximal Speed ◽

The Many ◽

Minimal Mass ◽

Novel Applications

Starting with a brief description of Born’s reciprocal relativity theory (BRRT), based on a maximal proper force, maximal speed of light, and inertial and non-inertial observers, we derive the exact thermal relativistic corrections to the Schwarzschild, Reissner–Nordstrom, and Kerr–Newman black hole entropies and provide a detailed analysis of the many novel applications and consequences to the physics of black holes, quantum gravity, minimal area, minimal mass, Yang–Mills mass gap, information paradox, arrow of time, dark matter, and dark energy. We finish by outlining our proposal towards a space–time–matter unification program where matter can be converted into spacetime quanta and vice versa.

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Black Hole Solution of Einstein-Born-Infeld-Yang-Mills Theory

Advances in High Energy Physics ◽

10.1155/2017/2038202 ◽

2017 ◽

Vol 2017 ◽

pp. 1-7 ◽

Cited By ~ 1

Author(s):

Kun Meng ◽

Da-Bao Yang ◽

Zhan-Ning Hu

Keyword(s):

Phase Transition ◽

Black Hole ◽

Phase Space ◽

Cosmological Constant ◽

Black Hole Solution ◽

Extended Phase Space ◽

Extended Phase ◽

Yang Mills ◽

First Law Of Thermodynamics ◽

Dimensional Black Hole

A new four-dimensional black hole solution of Einstein-Born-Infeld-Yang-Mills theory is constructed; several degenerated forms of the black hole solution are presented. The related thermodynamical quantities are calculated, with which the first law of thermodynamics is checked to be satisfied. Identifying the cosmological constant as pressure of the system, the phase transition behaviors of the black hole in the extended phase space are studied.

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