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相关论文: The Origin of Energy for the Big Bang

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The universe is filled with blackbody millimeter radiation (CMBR), temperature 2.7{\deg} Kelvin[1]. Big-bang cosmology explains this by the initial thermalization of photons scattered by electrons[2]. This explanation requires ad hoc…

综合物理 · 物理学 2010-04-14 Antonio Alfonso-Faus , Marius Josep Fullana i Alfonso

Our Universe has multiple examples of unexplained gravitational losses in black holes and neutron stars. As all of the space is squeezed out, nucleons are not easily compressible further. Gravitational loss will allow galactic black holes…

天体物理学 · 物理学 2024-12-24 David E. Rosenberg

The origins of matter and radiation in the universe lie in a Hot Big Bang. We present a number of well-motivated cosmologies in which the Big Bang occurs through a strong first order phase transition -- either at the end of inflation, after…

宇宙学与河外天体物理 · 物理学 2022-11-30 Katherine Freese , Martin Wolfgang Winkler

The big bang hypothesis is widely accepted despite numerous physics conflicts. It rests upon two experimental supports, galactic red shift and the cosmic microwave background. Both are produced by dark matter, shown here to be hydrogen…

综合物理 · 物理学 2008-03-31 Robert K. Soberman , Maurice Dubin

The standard model of cosmology assumes that our Universe began 14 Gyrs (billion years) ago from a singular Big Bang creation. This can explain a vast range of different astrophysical data from a handful of free cosmological parameters.…

宇宙学与河外天体物理 · 物理学 2022-04-26 Enrique Gaztanaga

The Hot Big Bang is often considered as the origin of all matter and radiation in the Universe. Primordial nucleosynthesis (BBN) provides strong evidence that the early Universe contained a hot plasma of photons and baryons with a…

宇宙学与河外天体物理 · 物理学 2023-05-03 Katherine Freese , Martin Wolfgang Winkler

Our universe has multiple examples of unexplained gravitational losses in black holes and neutron stars. The smallest black holes of about 4 solar masses means the maximum baryon density \rho \approx 10^{17} grams/cm^3. Any collapse of the…

天体物理学 · 物理学 2025-05-02 David E. Rosenberg

We speculate that the early Universe was inside a primordial black hole. The interior of the the black hole is a dS background and the two spacetimes are separated on the surface of black hole's event horizon. We argue that this picture…

高能物理 - 理论 · 物理学 2016-10-13 Hassan Firouzjahi

Rotating black holes are the most powerful source of energy in the known universe, and are the cause of some of the most spectacular and extreme astronomical phenomena. The goal of this article is to analyze in simple terms the physics of…

天体物理仪器与方法 · 物理学 2025-03-17 Jorge Pinochet

The total energy emitted by the growth of massive black holes is large and can be 10-50 per cent of that emitted by stars in the universe. I show how the X-ray Background provides a good measure of this energy and also why most accretion…

天体物理学 · 物理学 2009-10-31 A. C. Fabian

Black holes are a common feature of the Universe. They are observed as stellar mass black holes spread throughout galaxies and as supermassive objects in their centres. Observations of stars orbiting close to the centre of our Galaxy…

高能天体物理现象 · 物理学 2019-11-12 Andrew C. Fabian , Anthony N. Lasenby

If our universe was born as a baby universe on the other side of the event horizon of a black hole existing in a parent universe, then the corresponding white hole at rest provides the absolute frame of reference in the universe. In this…

科普物理 · 物理学 2025-06-02 Nikodem Popławski

A model for gravitational collapse where the event horizon is a quantum critical phase transition is extended to provide an explanation for the origin of the observable universe, where the expanding universe that we observe today was…

广义相对论与量子宇宙学 · 物理学 2016-02-09 George Chapline , James Barbieri

If even a relatively small number of black holes were created in the early universe, they will constitute an increasingly large fraction of the total energy density as space expands. It is thus well-motivated to consider scenarios in which…

高能物理 - 唯象学 · 物理学 2019-09-04 Dan Hooper , Gordan Krnjaic , Samuel D. McDermott

We propose that the totality of dark matter in the universe might ascribe its origin to one of the key properties of cosmological inflation, that it may be eternal: regions that at the end of the primordial accelerated expansion of the…

宇宙学与河外天体物理 · 物理学 2026-02-10 G. Franciolini , M. Peloso , A. Riotto

The thermal balance between the black hole and surrounding thermal radiation is an interesting topic. The primordial black hole is a type of black hole formed in the early universe, especially during the thermal radiation period of the…

广义相对论与量子宇宙学 · 物理学 2021-12-02 Ruifeng Zheng

Over the past three years we have determined the basic features of the Universe -- spatially flat; accelerating; comprised of 1/3 a new form of matter, 2/3 a new form of energy, with some ordinary matter and a dash of massive neutrinos; and…

天体物理学 · 物理学 2009-11-07 Michael S. Turner

I suggest the existence of a still undiscovered interaction: repulsion between matter and antimatter. The simplest and the most elegant candidate for such a force is gravitational repulsion between particles and antiparticles. I argue that…

综合物理 · 物理学 2011-02-10 Dragan Slavkov Hajdukovic

This paper develops a cosmological hypothesis based on the following propositions: 1. Zero-point radiation derives from quantic fluctuations in space, and the wavelength of its photons with the greatest energy is inversely proportional to…

综合物理 · 物理学 2007-06-26 R. Alvargonzalez , L. S. Soto

Black holes are extremely dense and compact objects from which light cannot escape. There is an overall consensus that black holes exist and many astronomical objects are identified with black holes. White holes were understood as the exact…

综合物理 · 物理学 2015-05-28 Alon Retter , Shlomo Heller
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