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We present a general polynomial chaotic inflation model in supergravity, for which the predicted spectral index and tensor-to-scalar ratio can lie within the 1 sigma region allowed by the Planck results. Most importantly, the predicted…

高能物理 - 唯象学 · 物理学 2015-06-16 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

Leptogenesis is the most favourable mechanism for generating the observed baryon asymmetry of the Universe (BAU) which implies CP violation in the high energy scale. The low energy leptonic CP violation is expected to be observed in the…

高能物理 - 唯象学 · 物理学 2015-06-16 H. Zeen Devi

We investigate dark matter (DM) phenomenology and cosmic inflation within a unified framework based on a dark $U(1)_D$ gauge extension of the Standard Model (SM). The associated dark gauge boson, namely the dark photon, serves as a viable…

高能物理 - 唯象学 · 物理学 2026-04-16 Sarif Khan , Jinsu Kim , Pyungwon Ko

We study slow roll single field inflationary scenario and the production of non-thermal fermionic dark matter, together with standard model Higgs, during reheating. For the inflationary scenario, we have considered two models of polynomial…

宇宙学与河外天体物理 · 物理学 2022-11-29 Anish Ghoshal , Gaetano Lambiase , Supratik Pal , Arnab Paul , Shiladitya Porey

Recent anomalies in cosmic rays could be due to dark matter annihilation in our galaxy. In order to get the required large cross-section to explain the data while still obtaining the right relic density, we rely on a non standard thermal…

高能物理 - 唯象学 · 物理学 2009-09-02 Bhaskar Dutta , Louis Leblond , Kuver Sinha

Phenomenological analysis to the R-parity violating supersymmetry with a vector-like extra generation is performed in detail. It is found that, via the trilinear couplings, the correct neutrino spectrum can be obtained. The Higgs mass rises…

高能物理 - 唯象学 · 物理学 2013-10-14 Xue Chang , Chun Liu , Yi-Lei Tang

The gravitino problem gives a severe constraint on the thermal leptogenesis scenario. This problem leads us to consider some alternatives to it if we try to keep the gravitino mass around the weak scale $m_{3/2} \sim 100$ GeV. We consider,…

高能物理 - 唯象学 · 物理学 2009-11-11 Takeshi Fukuyama , Tatsuru Kikuchi , Toshiyuki Osaka

We compute the gravitational leptogenesis generated from the parity-violating gravitational waves sourced by an abelian gauge field coupled to a pseudo-scalar inflation. We show that, once the CMB bound on the tensor-to-scalar ratio is…

宇宙学与河外天体物理 · 物理学 2017-12-20 Alexandros Papageorgiou , Marco Peloso

We study the evolution of matter density perturbations in Galileon cosmology where the late-time cosmic acceleration can be realized by a field kinetic energy. We obtain full perturbation equations at linear order in the presence of five…

宇宙学与河外天体物理 · 物理学 2011-02-23 Antonio De Felice , Ryotaro Kase , Shinji Tsujikawa

We discuss leptogenesis in a realistic supersymmetric model of inflation with a low reheat temperature 1-10 GeV. The lepton asymmetry is generated by a decaying right handed sneutrino, which is produced after inflation during preheating.…

高能物理 - 唯象学 · 物理学 2009-10-31 M. Bastero-Gil , S. F. King

We provide an anthropic reason that the supersymmetry breaking scale is much higher than the electroweak scale as indicated by the null result of collider experiments and observed 125 GeV Higgs boson. We focus on a new inflation model as a…

高能物理 - 唯象学 · 物理学 2016-03-23 Masahiro Kawasaki , Masaki Yamada , Tsutomu T. Yanagida , Norimi Yokozaki

Gravitinos are expected to be produced in any local supersymmetric model. Using their abundance prediction as a function of the reheating energy scale, it is argued that the next generation of Cosmic Microwave Background experiments could…

高能物理 - 唯象学 · 物理学 2009-11-10 A. Barrau , N. Ponthieu

We study the consequences of the gravitino decay into dark matter. We suppose that the lightest neutralino is the main component of dark matter. In our framework gravitino is heavy enough to decay before Big Bang Nucleosynthesis starts. We…

高能物理 - 唯象学 · 物理学 2007-06-29 David Gherson

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…

高能物理 - 唯象学 · 物理学 2013-01-16 Chee Sheng Fong , Enrico Nardi , Antonio Riotto

In the recently proposed `split supersymmetry' scenario, the squark and slepton masses are allowed to be at a high scale while the gauginos and Higgsinos are within a TeV. We show that in a theory with broken R-parity, the parameter space…

高能物理 - 唯象学 · 物理学 2010-04-05 Sudhir Kumar Gupta , Partha Konar , Biswarup Mukhopadhyaya

Current cosmological data seem to show that dark energy is evolving in time and that it possibly crossed the phantom divide in the past. So far the only theories that lead to such a behavior involve a non-trivial coupling between dark…

宇宙学与河外天体物理 · 物理学 2026-02-02 William J. Wolf , Pedro G. Ferreira , Carlos García-García

Leptogenesis scenarios in supersymmetric hybrid inflation models are considered. Sufficient lepton asymmetry leading to successful baryogenesis can be obtained if the reheat temperature T_r>10^6 GeV and the superpotential coupling parameter…

高能物理 - 唯象学 · 物理学 2008-11-26 V. N. Senoguz , Q. Shafi

In this work, we consider the gravitational baryogenesis in the framework of non-minimal derivative coupling model. A mechanism to generate the baryon asymmetry based on the coupling between the derivative of the Ricci scalar curvature and…

高能物理 - 理论 · 物理学 2023-11-06 Parviz Goodarzi

The Dirac nature of the gauginos (and also the Higgsinos) can be realized in $R$-symmetric supersymmetry models. In this class of models, the Dirac bino (or wino) with a small mixture of the Dirac Higgsinos is a good dark matter candidate.…

高能物理 - 唯象学 · 物理学 2011-03-22 Eung Jin Chun

In models with gauge mediated supersymmetry breaking the gravitino is the lightest supersymmetric particle. If R-parity is violated the gravitino decays, but with a half-live far exceeding the age of the universe and thus is, in principle,…

高能物理 - 唯象学 · 物理学 2008-11-26 M. Hirsch , W. Porod , D. Restrepo