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相关论文: Primordial Black Holes and Hot Matter

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Microscopic black holes explode with their temperature varying inversely as their mass. Such explosions would lead to the highest temperatures in the present universe, all the way to the Planck energy. Whether or not a quasi-stationary…

天体物理学 · 物理学 2008-11-26 J. I. Kapusta

The possibility that dark matter particles could be constituted by extreme regular primordial black holes is discussed. Extreme black holes have zero surface temperature, and are not subjected to the Hawking evaporation process. Assuming…

广义相对论与量子宇宙学 · 物理学 2018-05-14 José Antonio de Freitas Pacheco

The relativistic viscous fluid equations describing the outflow of high temperature matter created via Hawking radiation from microscopic black holes are solved numerically for a realistic equation of state. We focus on black holes with…

广义相对论与量子宇宙学 · 物理学 2009-11-07 R. G. Daghigh , J. I. Kapusta

About eight minutes before a black hole expires it has a decreasing mass of 10^{10} g, an increasing temperature of 1 TeV, and an increasing luminosity of 7x10^{27} erg/s. I show that such a black hole is surrounded by a quasi-stationary…

天体物理学 · 物理学 2007-05-23 Joseph Kapusta

Hawking radiation would make microscopic black holes evaporate rapidly, which excludes them from many astrophysical considerations. However, it has been argued that the quantum nature of space would alter this behaviour: the temperature of…

广义相对论与量子宇宙学 · 物理学 2021-11-05 Samuel Kováčik

The Hawking temperature for Schwarzschild black hole $T_H=1/8\pi M$ is singular in the limit of vanishing mass $M\to 0$. However, the Schwarzschild metric itself is regular in this limit, it is reduced to the Minkowski metric and there are…

高能物理 - 理论 · 物理学 2021-04-27 Irina Aref'eva , Igor Volovich

We consider the early universe at temperatures close to the fundamental scale of gravity (M_D << M_Planck) in models with extra dimensions. At such temperatures a small fraction of particles will experience transplanckian collisions that…

高能物理 - 理论 · 物理学 2010-01-26 Monica Borunda , Manuel Masip

The Hawking evaporation of primordial black holes (PBH) reheats the Universe locally, forming hot spots that survive throughout their lifetime. We propose to use the temperature profile of such hot spots to calculate the decay rate of…

高能物理 - 唯象学 · 物理学 2024-10-15 Louis Hamaide , Lucien Heurtier , Shi-Qian Hu , Andrew Cheek

We investigate models in which a spectrum of black holes with Hawking temperature of order the radiation temperature at the beginning of the radiation dominated era can survive long enough to produce a matter dominated era at the observed…

高能物理 - 理论 · 物理学 2020-08-04 Tom Banks , Willy Fischler

Many early universe theories predict the creation of Primordial Black Holes (PBHs). The PBHs could have masses ranging from the Planck mass to 10^5 solar masses or higher depending on the formation scenario. Hawking showed that any Black…

高能天体物理现象 · 物理学 2015-11-02 J. T. Linnemann , D. Stump , S. S. Marinelli , T. Yapici , K. Tollefson , T. N. Ukwatta , J. H. MacGibbon

We show that primordial (nearly) extremal black holes with a wide range of masses from the Planck scale to around $10^9$ g could be cosmologically stable and explain dark matter, given a dark electromagnetism and a heavy dark electron. For…

高能物理 - 唯象学 · 物理学 2020-03-11 Yang Bai , Nicholas Orlofsky

Primordial black holes are a viable dark matter candidate. They decay via Hawking evaporation. Energetic particles from the Hawking radiation interact with interstellar gas, depositing their energy as heat and ionization. For a sufficiently…

高能物理 - 唯象学 · 物理学 2021-05-12 Hyungjin Kim

Two interesting hypotheses about black holes have been proposed. The older one states that microscopic black holes can be accountable for the observed dark matter density. The newer one states that black holes are coupled to the expansion…

广义相对论与量子宇宙学 · 物理学 2024-05-24 Samuel Kováčik

If the temperature of the hot thermal plasma in the Early Universe was within a few orders of magnitude of the Planck scale $M_{\rm Pl}$, then the hoop conjecture predicts the formation of microscopic black holes from particle collisions in…

高能物理 - 唯象学 · 物理学 2023-10-03 Avi Friedlander , Ningqiang Song , Aaron C. Vincent

Primordial black holes (PBHs) with mass $10^{16}-10^{17}$ g almost escape constraints from observations so could essentially contribute to dark matter density. Hawking evaporation of such PBHs produces with a steady rate $\gamma$- and…

宇宙学与河外天体物理 · 物理学 2015-02-26 K. M. Belotsky , A. A. Kirillov

We have computed the thermodynamic properties of a rotating black holes in the presence of cold dark matter. The dependence of temperaure, Gibbs free energy, specific heat on the horizon radius have been studied for various values of…

广义相对论与量子宇宙学 · 物理学 2024-09-10 Swapan Kumar Majhi

Many early universe theories predict the creation of Primordial Black Holes (PBHs). PBHs could have masses ranging from the Planck mass to 10^5 solar masses or higher depending on the size of the universe at formation. A Black Hole (BH) has…

高能天体物理现象 · 物理学 2016-04-27 T. N. Ukwatta , D. R. Stump , J. T. Linnemann , J. H. MacGibbon , S. S. Marinelli , T. Yapici , K. Tollefson

Vilkovisky has claimed to have solved the black hole backreaction problem and finds that black holes lose only ten percent of their mass to Hawking radiation before evaporation ceases. We examine the implications of this scenario for cold…

宇宙学与河外天体物理 · 物理学 2012-12-10 Julien Larena , Tony Rothman

Primordial Black Holes (PBHs) are black holes that may have been created in the early Universe and could be as large as supermassive black holes or as small as the Planck scale. It is believed that a black hole has a temperature inversely…

高能天体物理现象 · 物理学 2015-08-17 T. N. Ukwatta , J. T. Linnemann , D. Stump J. H. MacGibbon , S. S. Marinelli , T. Yapici , K. Tollefson

Recently, a new framework for solving the hierarchy problem was proposed which does not rely on low energy supersymmetry or technicolor. The fundamental Planck mass is at a TeV and the observed weakness of gravity at long distances is due…

高能物理 - 理论 · 物理学 2009-10-31 Philip C. Argyres , Savas Dimopoulos , John March-Russell
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