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Related papers: Proton decay in de Sitter environment

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The existing thermodynamics of the cosmological horizon in de-Sitter spacetime is established in the micro-canonical ensemble, while thermodynamics of black hole horizons are established in the canonical ensemble. Generally in the ordinary…

General Relativity and Quantum Cosmology · Physics 2013-11-05 Hiromi Saida

It is well known that de Sitter(dS) black holes generally have a black hole horizon and a cosmological horizon, both of which have Hawking radiation. But the radiation temperature of the two horizons is generally different, so dS black…

High Energy Physics - Theory · Physics 2021-02-03 Yubo Ma , Yang Zhang , Lichun Zhang , Liang Wu , Ying Gao , Shuo Cao , Yu Pan

Increasing the spin coherence time (T2) is a major area of interest for spin defect systems such as the silicon (V$_Si$) and carbon (V$^\pm _C$) vacancies in 4H-SiC. Usually as temperature increases, T2 decreases due to the thermal bath.…

Mesoscale and Nanoscale Physics · Physics 2025-10-02 P. Chrostoski , Ifeanyi I. Onwosi , D. H. Santamore

Though the problem of Hawking radiation in de Sitter space-time, in particular details of penetration of a quantum mechanical particle through the de Sitter horizon, has been examined intensively there is still some vagueness in this…

Mathematical Physics · Physics 2012-11-20 V. Red'kov , E. Ovsiyuk , G. Krylov

The mechanism of decoherence for a quantum system with rotational degrees of freedom is studied. From a simple model of elastic scattering, we show that the non-diagonal density matrix elements of the system exponentially decay. The decay…

Quantum Physics · Physics 2016-11-18 Changchun Zhong , F. Robicheaux

We study scalar particle decay during the radiation and matter dominated epochs of a standard cosmological model. An adiabatic approximation is introduced that is valid for degrees of freedom with typical wavelengths much smaller than the…

High Energy Physics - Phenomenology · Physics 2018-10-03 Nathan Herring , Brian Pardo , Daniel Boyanovsky , Andrew R. Zentner

A central problem of space plasma physics is how protons and electrons are heated in a turbulent, magnetized plasma. The differential heating of charged species due to dissipation of turbulent fluctuations plays a key role in solar wind…

We rephrase the derivation of black hole radiation so as to take into account, at the level of transition amplitudes, the change of the geometry induced by the emission process. This enlarged description reveals that the dynamical variables…

General Relativity and Quantum Cosmology · Physics 2009-10-31 S. Massar , R. Parentani

We consider the minimal supersymmetric SO(10) model, where only one {\bf 10} and one $\bar{\bf 126}$ Higgs multiplets have Yukawa couplings with matter multiplets. This model has the high predictive power for the Yukawa coupling matrices…

High Energy Physics - Phenomenology · Physics 2008-11-26 Takeshi Fukuyama , Amon Ilakovac , Tatsuru Kikuchi , Stjepan Meljanac , Nobuchika Okada

In this paper, we discuss the tunneling of scalar particles near the event horizon of stationary and nonstationary Kerr-de Sitter black hole using Lorentz violation theory in curved space time. The modified form of Hamilton-Jacobi equation…

General Relativity and Quantum Cosmology · Physics 2023-01-03 Y. Onika Laxmi , T. Ibungochouba Singh

Due to a well-known, but curious, minus sign in the Gibbons-Hawking first law for the static patch of de Sitter space, the entropy of the cosmological horizon is reduced by the addition of Killing energy. This minus sign raises the puzzling…

High Energy Physics - Theory · Physics 2023-09-08 Batoul Banihashemi , Ted Jacobson , Andrew Svesko , Manus Visser

Vacuum decay in de Sitter space is a process of great physical interest, as it allows to rule out cosmological models in the early and current Universe. Its rate may be described in terms of an instanton in Euclidean space called bounce and…

General Relativity and Quantum Cosmology · Physics 2022-05-24 Silvia Vicentini

The effect of the Hawking temperature on the entanglement and teleportation for the scalar field in a most general, static and asymptotically flat black hole with spherical symmetry has been investigated. It is shown that the same "initial…

General Relativity and Quantum Cosmology · Physics 2009-02-20 Qiyuan Pan , Jiliang Jing

In this paper we focus on the gravitational thermodynamics of the far future. Cosmological observations suggest that most matter will be diluted away by the cosmological expansion, with the rest collapsing into supermassive black holes. The…

General Relativity and Quantum Cosmology · Physics 2012-01-09 Andrew P. Lundgren , Mihai Bondarescu , Ruxandra Bondarescu

The mean kinetic energy of protons in water is determined by Deep Inelastic Neutron Scattering experiments, performed above and below the temperature of maximum density and in the supercooled phase. The temperature dependence of this energy…

Soft Condensed Matter · Physics 2015-05-13 Davide Flammini , Fabio Bruni , Maria Antonietta Ricci

When primordial black holes (PBHs) evaporate, they deposit energy in the surrounding plasma, leading to temperature gradients, or hot spots, that evolve during the evaporation process. Motivated by recent studies suggesting that a memory…

Cosmology and Nongalactic Astrophysics · Physics 2025-11-24 Nathaniel Levy , Lucien Heurtier

The temperature of the atomic matter in the Universe is held to that of the Cosmic Background radiation until decoupling at z~100. After this it cools faster than the radiation (\propto(1+z)^2 rather than (1+z)) and would have fallen to…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 Douglas Scott , Adam Moss

The temperature dependence of hydrogen (H) desorption from Si(100) H-terminated surfaces by a scanning tunneling microscope (STM) is reported for negative sample bias. It is found that the STM induced H desorption rate ($R$) decreases…

Materials Science · Physics 2009-10-31 C. Thirstrup , M. Sakurai , T. Nakayama , K. Stokbro

The change in the decay rate of an excited atom that is brought about by extinction and thermal-radiation effects in a nearby dielectric medium is determined from a quantummechanical model. The medium is a collection of randomly distributed…

Quantum Physics · Physics 2018-07-23 L. G. Suttorp , A. J. van Wonderen

The finite temperature and finite density dependence of the neutron-proton mass difference is analysed in a purely hadronic framework where the $\rho-\omega $ mixing is crucial for this isospin symmetry breakdown. The problem is handled…

High Energy Physics - Phenomenology · Physics 2016-08-15 H. R. Christiansen , L. N. Epele , H. Fanchiotti , C. A. García Canal
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