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Related papers: The $\nu$MSM, Inflation, and Dark Matter

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The tiny neutrino masses are most naturally explained by seesaw mechanism through singlet right-handed neutrinos, which can further explain the matter-antimatter asymmetry in the Universe. In this Letter, we propose a new approach to study…

High Energy Physics - Phenomenology · Physics 2025-11-05 Chengcheng Han , Hong-Jian He , Linghao Song , Jingtao You

We consider a supersymmetric model of inflation in which the primordial density fluctuations are nearly scale invariant (the spectral index n is approximately 0.98) with amplitude proportional to (M/M_{Planck})^2, where M ~ 10^{16} GeV…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Lazarides , R. K. Schaefer , Q. Shafi

The similarity of the observed densities of baryons and cold dark matter suggests that they have a common or related origin. This can be understood in the context of the MSSM with right-handed (RH) sneutrinos if cold dark matter is due to a…

High Energy Physics - Phenomenology · Physics 2010-10-27 John McDonald

We investigate the Two-Higgs-Doublet-Standard Model-Axion-Seesaw-Higgs-Portal inflation (2hdSMASH) model consisting of two Higgs doublets, a Standard Model (SM) singlet complex scalar and three SM singlet right-handed Majorana neutrinos…

High Energy Physics - Phenomenology · Physics 2023-12-22 Juhi Dutta

We study the inflation due to the D-flat direction of an extra $U(1)$. This scenario is a hybrid of a right-handed sneutrino inflaton scenario and a gauge non-singlet inflaton scenario. The inflaton is a gauge non-singlet field which…

High Energy Physics - Phenomenology · Physics 2009-10-28 Daijiro Suematsu , Yoshio Yamagishi

Superheavy dark matter has been attractive as a candidate of particle dark matter. We propose a ``natural" particle model, in which the dark matter serves as the inflaton in natural inflation, while decaying to high-energy particles at…

High Energy Physics - Phenomenology · Physics 2025-12-03 Kohta Murase , Yuma Narita , Wen Yin

The discrete symmetry $Z_4$ in the standard model (SM) with three right-handed neutrinos is free from the Dai-Freed anomaly. Motivated by this $Z_4$ symmetry, we constructed a topological inflation model consistent with all known…

High Energy Physics - Phenomenology · Physics 2023-06-27 Masahiro Kawasaki , Tsutomu T. Yanagida

In a previous paper, we proposed a simple extension of the Minimal Supersymmetric Standard Model which gives rise to thermal inflation and baryogenesis in a natural and remarkably consistent way. In this paper, we consider the $\lambda_\phi…

High Energy Physics - Phenomenology · Physics 2009-02-12 Seongcheol Kim , Wan-Il Park , Ewan D. Stewart

We present a complete particle physics model that explains three major problems of modern cosmology: inflation, dark matter and dark energy, and also gives a mechanism for leptogenesis. The model has a new gauge group $SU(2)_Z$ that grows…

Astrophysics · Physics 2008-11-26 P. Q. Hung , Eduard Masso , Gabriel Zsembinszki

We present here the effective theory of inflation `a la Ginsburg-Landau in which the inflaton potential is a polynomial. The slow-roll expansion becomes a systematic 1/N expansion where N ~ 60. The spectral index and the ratio of…

Cosmology and Nongalactic Astrophysics · Physics 2010-06-24 H. J. de Vega

The seesaw mechanism with three heavy Majorana right-handed neutrinos provides an elegant explanation for neutrino masses and, combined with leptogenesis, can generate the baryon asymmetry of the universe (BAU). Naturally embedded in a…

High Energy Physics - Phenomenology · Physics 2025-05-06 Juan Herrero-Garcia , Giacomo Landini , Tsutomu T. Yanagida

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

We present a new approach to quintessential inflation, in which both dark energy and inflation are explained by the evolution of a single scalar field. We start from a simple scalar potential with both oscillatory and exponential…

High Energy Physics - Phenomenology · Physics 2007-05-23 Gabriela Barenboim

We study an inflection point inflation scenario where a flat direction of the minimal supersymmetric standard model (MSSM) is identified with the inflaton. We focus on the case where the flat direction (inflaton) has non-zero baryon number,…

High Energy Physics - Phenomenology · Physics 2024-10-17 Naoyuki Haba , Yasuhiro Shimizu , Yoshihiro Tanabe , Toshifumi Yamada

We propose a model of inflation driven by minimal extension of SUSY, commonly known as MSSM. Starting from gauge invariant flat directions in the n = 4 level comprising of QQQL,QuQd,QuLe and uude, we construct the inflaton potential and…

High Energy Physics - Phenomenology · Physics 2012-04-19 Sayantan Choudhury , Supratik Pal

It is shown that in the phenomenologically realistic supersymmetric $B-L$ MSSM theory, a linear combination of the neutral, up Higgs field with the third family left-and right-handed sneutrinos can play the role of the cosmological…

High Energy Physics - Phenomenology · Physics 2017-02-15 Rehan Deen , Burt A. Ovrut , Austin Purves

In a previous paper, the standard model was generalized to include an electroweak axion which carries baryon plus lepton number, $B+L$. It was shown that such a model naturally gives the observed value of the dark energy, if the scale of…

High Energy Physics - Phenomenology · Physics 2015-06-23 Larry McLerran

We propose a novel reformulation of supersymmetric (more precisely $\mu$-) hybrid inflation based on a local U(1) or any suitable extension of the minimal supersymmetric standard model (MSSM) which also resolves the $\mu$ problem. We employ…

High Energy Physics - Phenomenology · Physics 2018-11-14 Nobuchika Okada , Qaisar Shafi

In the minimal gauged B-L extension of the Standard Model, we demonstrate that PeV-scale dark matter (DM) and the baryon asymmetry of the Universe (BAU) can be simultaneously explained through the three right-handed neutrinos (RHNs) present…

High Energy Physics - Phenomenology · Physics 2025-08-05 Basabendu Barman , Arindam Das , Suruj Jyoti Das , Marco Merchand

We present a minimal model for particle physics and cosmology. The Standard Model (SM) particle content is extended by three right-handed SM-singlet neutrinos N_i and a vector-like quark Q, all of them being charged under a global lepton…

High Energy Physics - Phenomenology · Physics 2016-10-18 Andreas Ringwald
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