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Related papers: Scenario of baryogenesis

200 papers

We present the evidence that crossover, fluctuation phenomena and possible Anderson transition are the precursors of quark matter formation.

High Energy Physics - Phenomenology · Physics 2008-11-26 B. Kerbikov , E. V. Luschevskaya

We propose an alternative mechanism of baryogenesis in which a scalar baryon undergoes a percolating first-order phase transition in the early Universe. The potential barrier that divides the phases contains explicit B and CP violation and…

High Energy Physics - Phenomenology · Physics 2015-06-05 Clifford Cheung , Alex Dahlen , Gilly Elor

Additional elementary species and primordial black holes are common candidates for dark matter. Their co-existence in the early Universe leads to accretion if particles are heavy. We solve equation of motion affected by expansion which…

Cosmology and Nongalactic Astrophysics · Physics 2025-03-25 N. A. Pozdnyakov

We study the possibility that partonic matter produced at early stage of ultrarelativistic heavy-ion collisions is out of chemical equilibrium. It is assumed that initially this matter is mostly composed of gluons, but quarks and antiquarks…

High Energy Physics - Phenomenology · Physics 2016-01-21 V. Vovchenko , M. I. Gorenstein , L. M. Satarov , I. N. Mishustin , L. P. Csernai , I. Kisel , H. Stoecker

Planet formation occurs within the gas and dust rich environments of protoplanetary disks. Observations of these objects show that the growth of primordial sub micron sized particles into larger aggregates occurs at the earliest stages of…

Earth and Planetary Astrophysics · Physics 2015-06-11 Pascale Garaud , Farzana Meru , Marina Galvagni , Christoph Olczak

The properties of the first-order phase transition in a set of plasma models with common feature - absence of individual correlations between charges of op-posite sign, have been studied. Predicted discontinuities in equilibrium non-uniform…

Plasma Physics · Physics 2007-05-23 Igor L. Iosilevski , Alexander Yu. Chigvintsev

For a brief time in its early evolution the Universe was a cosmic nuclear reactor. The expansion and cooling of the Universe limited this epoch to the first few minutes, allowing time for the synthesis in astrophysically interesting…

Cosmology and Nongalactic Astrophysics · Physics 2010-09-27 Gary Steigman

We discuss the chemical pre-conditions for planet formation, in terms of gas and ice abundances in a protoplanetary disk, as function of time and position, and the resulting chemical composition and cloud properties in the atmosphere when…

Earth and Planetary Astrophysics · Physics 2014-06-25 Ch. Helling , P. Woitke , P. B. Rimmer , I. Kamp , W. -F. Thi , R. Meijerink

A system H with a Hagedorn-like mass spectrum imparts its unique temperature T_H to any other system coupled to it. An H system radiates particles in preexisting physical and chemical equilibrium. These particles form a saturated vapor at…

High Energy Physics - Phenomenology · Physics 2007-05-23 L. G. Moretto , K. A. Bugaev , J. B. Elliott , L. Phair

We argue that the creation of a baryon asymmetry in the early universe is an intriguing case where several aspects of ``Beyond'' physics are needed. We then concentrate on baryogenesis in a strong first-order phase transition and discuss…

High Energy Physics - Phenomenology · Physics 2014-11-17 Michael G. Schmidt

Assuming that vector and scalar diquarks exist in the Quark-Gluon Plasma near the critical temporature $T_c$, baryons can be produced through the processes of quarks and diquarks forming $({1/2})^+$ baryon states. Ratios of different…

High Energy Physics - Phenomenology · Physics 2008-11-26 Hong Miao , Zhongbiao Ma , Chongshou Gao

We demonstrate the viability of electroweak baryogenesis scenarios in which the necessary departure from equilibrium is realized by the evolution of a network of topological defects. We consider several effective models of TeV physics, each…

High Energy Physics - Phenomenology · Physics 2010-11-01 M. Trodden , A-C. Davis , R. Brandenberger

If inflaton couples very weakly to ordinary matter the reheating temperature of the universe can be lower than the electroweak scale. In this letter we show that the late reheating occurs in a highly non-uniform way, within narrow areas…

High Energy Physics - Phenomenology · Physics 2009-11-10 Takehiko Asaka , Dmitri Grigoriev , Vadim Kuzmin , Mikhail Shaposhnikov

After some introductory remarks about the prospects of first order phase transitions in the early universe, we discuss in some detail the electroweak phase transition. In the standard model case a clear picture is arising including…

High Energy Physics - Phenomenology · Physics 2007-05-23 M. G. Schmidt

Leptogenesis is a class of scenarios in which the cosmic baryon asymmetry originates from an initial lepton asymmetry generated in the decays of heavy sterile neutrinos in the early Universe. We explain why leptogenesis is an appealing…

High Energy Physics - Phenomenology · Physics 2013-01-16 Chee Sheng Fong , Enrico Nardi , Antonio Riotto

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…

High Energy Physics - Theory · Physics 2010-01-26 Monica Borunda , Manuel Masip

In thermal equilibrium the ground state of the plasma of Standard Model particles is determined by temperature and exactly conserved combinations of baryon and lepton numbers. We show that at non-zero values of the global charges a…

High Energy Physics - Phenomenology · Physics 2012-10-09 Alexey Boyarsky , Oleg Ruchayskiy , Mikhail Shaposhnikov

The question of a phase transition in exiting the Planck epoch of the early universe is addressed. An order parameter is proposed to help decide the issue, and estimates are made concerning its behavior. Our analysis is suggestive that a…

General Relativity and Quantum Cosmology · Physics 2009-10-31 Stuart Samuel

An essential prerequisite for quark-gluon plasma production in nuclear collisions is cross-talk between the partons from different nucleons in the colliding nuclei. The initial density of partons is determined by the parton distribution…

High Energy Physics - Phenomenology · Physics 2007-05-23 H. Satz

Volatiles are compounds with low sublimation temperatures, and they make up most of the condensible mass in typical planet-forming environments. They consist of relatively small, often hydrogenated, molecules based on the abundant elements…

Earth and Planetary Astrophysics · Physics 2015-06-18 Klaus M. Pontoppidan , Colette Salyk , Edwin A. Bergin , Sean Brittain , Bernard Marty , Olvier Mousis , Karin L. Oberg
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