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In this letter, we quantify the challenge of explaining the baryon asymmetry using initial conditions in a universe that undergoes inflation. Contrary to lore, we find that such an explanation is possible if net $B-L$ number is stored in a…

High Energy Physics - Phenomenology · Physics 2017-09-06 Gordan Krnjaic

We consider the creation of the cosmological baryon asymmetry in the Two Higgs Doublet Model. We imagine a situation where the masses of the five Higgs particles and the two Higgs vevs are constrained by collider experiments, and…

High Energy Physics - Phenomenology · Physics 2015-06-11 Anders Tranberg , Bin Wu

We propose a minimal and motivated extension of the Standard Model characterised by an approximate lepton number conservation, which is able to simultaneously generate neutrino masses and to account for a successful baryogenesis via…

High Energy Physics - Phenomenology · Physics 2016-08-24 Michele Lucente , Asmaa Abada , Giorgio Arcadi , Valerie Domcke

In order to address the baryon asymmetry in the Universe one needs to understand the origin of baryon (B) and lepton (L) number violation. In this article, we discuss the mechanism of baryogenesis via leptogenesis to explain the…

High Energy Physics - Phenomenology · Physics 2021-09-10 Pavel Fileviez Perez , Clara Murgui , Alexis D. Plascencia

In this paper, to be closer to the realities of the relativistic heavy ion collisions than the thermal equilibrium assumption often used in the calculations of baryon number susceptibilities, the creatures of the collisions are treated as…

High Energy Physics - Phenomenology · Physics 2021-07-08 Ameng Zhao

We show that a baryon asymmetry can be generated by dissipative effects during warm inflation via a supersymmetric two-stage mechanism, where the inflaton is coupled to heavy mediator fields that then decay into light species through B- and…

High Energy Physics - Phenomenology · Physics 2015-05-30 Mar Bastero-Gil , Arjun Berera , Rudnei O. Ramos , Joao G. Rosa

Within a supersymmetric (SUSY) type-I seesaw framework with flavor-blind universal boundary conditions, we study the consequences of requiring that the observed baryon asymmetry of the Universe be explained by either thermal or non-thermal…

High Energy Physics - Phenomenology · Physics 2010-11-15 Steve Blanchet , Danny Marfatia , Azar Mustafayev

In the following work we consider the possibility of explaining the observed baryon number asymmetry in the universe from simple baryon number violating modifications, involving massive scalar bosons, to the Standard Model. In these cases…

High Energy Physics - Phenomenology · Physics 2009-10-30 J. P. Bowes , R. R. Volkas

In $E_6$ models there are new particles whose baryon number is not uniquely assigned. We point out that the baryon and lepton number assignment to these particles can change the baryogenesis scenario significantly. We consider left-right…

High Energy Physics - Phenomenology · Physics 2009-10-28 Emmanuel A. Paschos , Utpal Sarkar , Hiroto So

Fluctuations of scalar fields produced at the stage of preheating after inflation are so large that they can break supersymmetry much stronger than inflation itself. These fluctuations may lead to symmetry restoration along flat directions…

High Energy Physics - Phenomenology · Physics 2009-09-29 Greg. W. Anderson , Andrei Linde , Antonio Riotto

I show that a cosmological baryon asymmetry generated at the GUT scale is in general safe against washout due to sphalerons and generic $B$- or $L$-violating effects. This result is mainly due to the (almost) conserved number of…

High Energy Physics - Phenomenology · Physics 2010-11-01 Kimmo Kainulainen

We discuss the relation between lepton number violation at high and low energies, particularly, the constraints on baryogenesis models, which would be implied by an observation of neutrinoless double beta decay. The primordial baryon…

High Energy Physics - Phenomenology · Physics 2016-05-05 Lukas Graf

We consider the evolution of baryon number $B$ in the early universe under the influence of rapid sphaleron interactions and show that $B$ will remain nonzero at all times even in the case of $B-L = 0$. This result arises due to thermal…

High Energy Physics - Phenomenology · Physics 2009-09-15 S. Davidson , K. Kainulainen , K. A. Olive

We consider a conformal unified theory as the basis of conformal-invariant cosmological model where the permanent rigid state of the universe is compatible with the primordial element abundance and supernova data. We show that the…

High Energy Physics - Theory · Physics 2007-05-23 D. Blaschke , A. Gusev , V. Pervushin , D. Proskurin

The Standard Model accompanied with two right-handed neutrinos with the masses below the weak scale can explain the observed baryon asymmetry of the Universe. Moreover, this model is at least partially testable in the forthcoming…

High Energy Physics - Phenomenology · Physics 2019-10-23 Shintaro Eijima , Mikhail Shaposhnikov , Inar Timiryasov

In a dynamical model of QGP at RHIC we obtain the temporal evolution of strange phase space occupancy at conditions expected to occur in 100+100A GeV nuclear collisions. We show that the sudden QGP break up model developed to describe the…

Nuclear Theory · Physics 2009-10-31 Johann Rafelski , Jean Letessier

The correlation between baryon number and strangeness is used to discern the nature of the deconfined matter produced at vanishing chemical potential in high-energy nuclear collisions at the BNL RHIC. Comparisons of results of various…

Nuclear Theory · Physics 2009-11-11 A. Majumder , V. Koch , J. Randrup

This talk is based on work performed with Graham Ross and is a very concise summary of our soon to be published paper. Here we present a revision of the analysis of sphaleron baryon-number violating processes in the standard model including…

High Energy Physics - Phenomenology · Physics 2007-05-23 Herbi Dreiner

The observational relation between the density of baryon and dark matter in the Universe, $\Omega_{\rm DM}/\Omega_B\simeq 5$, is one of the most difficult problems to solve in modern cosmology. We discuss a scenario that explains this…

High Energy Physics - Phenomenology · Physics 2013-05-30 Kohei Kamada , Masahide Yamaguchi

We consider a model in which dark matter is a composite baryon of a dark sector governed by $SU(3)$ gauge theory, with vector-like quarks also charged under $U(1)_Y$. The model provides simple answer to the dark matter stability problem: it…

High Energy Physics - Phenomenology · Physics 2016-10-21 Ran Huo , Shigeki Matsumoto , Yue-Lin Sming Tsai , Tsutomu T. Yanagida
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