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Related papers: Flux-Induced Baryon Asymmetry

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Scalar fields in the minimal supersymmetric standard model may have large field values during inflation. Because of approximate global symmetry, it is plausible that the phase directions of them are nearly massless during inflation and…

High Energy Physics - Phenomenology · Physics 2020-12-30 Keisuke Harigaya , Masaki Yamada

The baryon asymmetry of the universe may be explained by rotations of the QCD axion in field space and baryon number violating processes. We consider the minimal extension of the Standard Model by a non-Abelian gauge interaction, $SU(2)_R$,…

High Energy Physics - Phenomenology · Physics 2021-12-24 Keisuke Harigaya , Isaac R. Wang

We explore the possibility that the observed baryon asymmetry of the universe is the result of an earlier phase transition in which an extended gauge sector breaks down into the $SU(3)_C \times SU(2)_L \times U(1)_Y$ of the Standard Model.…

High Energy Physics - Phenomenology · Physics 2008-11-26 Jing Shu , Tim M. P. Tait , Carlos E. M. Wagner

In theories where $B-L$ is a spontaneously broken local symmetry, the cosmological baryon asymmetry can be generated by the out-of-equilibrium decay of heavy Majorana neutrinos. We study this mechanism assuming a similar pattern of mixings…

High Energy Physics - Phenomenology · Physics 2009-10-28 W. Buchmuller , M. Plumacher

In this work, we explain three beyond standard model (BSM) phenomena, namely neutrino masses, the baryon asymmetry of the Universe and Dark Matter, within a single model and in each explanation the right handed (RH) neutrinos play the prime…

High Energy Physics - Phenomenology · Physics 2019-06-26 Anirban Biswas , Sandhya Choubey , Laura Covi , Sarif Khan

One of the most efficient mechanisms for producing the baryon asymmetry of the Universe is the decay of scalar condensates in a SUSY GUT as was first suggested by Affleck and Dine. We show that given a large enough asymmetry, the baryon…

High Energy Physics - Phenomenology · Physics 2009-09-15 Sacha Davidson , Hitoshi Murayama , Keith A. Olive

The similar cosmological abundances observed for visible and dark matter suggest a common origin for both. By viewing the dark matter density as a dark-sector asymmetry, mirroring the situation in the visible sector, we show that the…

High Energy Physics - Phenomenology · Physics 2012-03-01 Kalliopi Petraki , Mark Trodden , Raymond R. Volkas

It has been pointed out that hypermagnetic helicity decay at the electroweak symmetry breaking may have produced the observed baryon asymmetry of the Universe through the chiral anomaly in the standard model of particle physics. Although…

Cosmology and Nongalactic Astrophysics · Physics 2021-04-21 Kohei Kamada , Fumio Uchida , Jun'ichi Yokoyama

One of the most experimentally testable explanations for the origin of the baryon asymmetry of the universe is that it was created during the electroweak phase transition, in the minimal supersymmetric standard model. Previous efforts have…

High Energy Physics - Phenomenology · Physics 2008-11-26 James M. Cline , Kimmo Kainulainen

We propose that the baryon asymmetry of the Universe may originate from the amplification of quantum fluctuations of a light complex scalar field during inflation. CP-violation is sourced by complex mass terms, which are smaller than the…

Astrophysics · Physics 2008-12-18 Bjorn Garbrecht , Tomislav Prokopec

In this work we review the theories of origin of matter-antimatter asymmetry in the Universe. The general conditions for achieving baryogenesis and leptogenesis in a CPT conserving field theory have been laid down by Sakharov. In this…

High Energy Physics - Phenomenology · Physics 2015-06-17 G. Lambiase , S. Mohanty , A. R. Prasanna

We have shown that the $B-L$ generation due to the decay of the thermally produced superheavy fields can explain the Baryon assymmetry in the universe if the superheavy fields are heavier than $10^{13-14}$ GeV. Note that although the…

High Energy Physics - Phenomenology · Physics 2013-05-29 Seishi Enomoto , Nobuhiro Maekawa

Baryon asymmetry of the universe is generated in the supersymmetric standard model (SSM) through the charge transport mechanism mediated by top squarks. Necessary CP violation originates from a complex phase contained in mass-squared…

High Energy Physics - Phenomenology · Physics 2007-05-23 Mayumi Aoki , Noriyuki Oshimo

The present matter content of our universe may be governed by a $U(1)_{B-L}$ symmetry -- the simplest gauge completion of the seesaw mechanism which produces small neutrino masses. The matter parity results as a residual gauge symmetry,…

High Energy Physics - Phenomenology · Physics 2020-12-15 Phung Van Dong , Duong Van Loi

It has been recently speculated that global symmetries are broken by gravity. We propose a scenario for the generation of the baryon asymmetry in the early Universe in which the domain walls predicted by theories with discrete symmetries…

High Energy Physics - Phenomenology · Physics 2009-10-22 H. Lew , A. Riotto

Stringent bounds on baryon and lepton number violating interactions have been derived from the requirement that such interactions, together with electroweak instantons, do not destroy a cosmological baryon asymmetry produced at an extremely…

High Energy Physics - Phenomenology · Physics 2009-10-22 Aram Antaramian , Lawrence J. Hall , Andrija Rašin

We show that the baryon asymmetry of the Universe cannot be explained by a large initial value before inflation because it inevitably predicts correlated baryon isocurvature perturbations that are already excluded by cosmic microwave…

Cosmology and Nongalactic Astrophysics · Physics 2023-07-07 Kai Murai , Fuminobu Takahashi , Masaki Yamada , Wen Yin

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 the presence of anomaly induced sphaleron process, only a B-L asymmetry can be partially converted to the baryon asymmetry while any B+L asymmetry would be completely erased. Thus in any successful baryogenesis theories, B-L is usually…

High Energy Physics - Phenomenology · Physics 2008-11-26 Pei-Hong Gu , Utpal Sarkar

We calculate the baryon asymmetry of the Universe which would arise during a first order electroweak phase transition due to minimal standard model processes. It agrees in sign and magnitude with the observed baryonic excess, for resonable…

High Energy Physics - Phenomenology · Physics 2010-11-01 Glennys R. Farrar , M. E. Shaposhnikov