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相关论文: Generating Luminous and Dark Matter During Inflati…

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We construct supersymmetric unified models which automatically lead to a period of inflation. The models all involve a U(1) symmetry which does not belong to the MSSM. We consider three different types of models depending on whether this…

高能物理 - 唯象学 · 物理学 2009-10-30 R. Jeannerot

We propose a model with an $U(1)_{B-L}$ gauge symmetry, in which small neutrino masses, dark matter and the matter-antimatter asymmetry in the Universe can be simultaneously explained. In particular, the neutrino masses are generated…

高能物理 - 唯象学 · 物理学 2018-02-19 Chao-Qiang Geng , Hiroshi Okada

We show how to enlarge the $\nu$MSM (the minimal extension of the standard model by three right-handed neutrinos) to incorporate inflation and provide a common source for electroweak symmetry breaking and for right-handed neutrino masses.…

高能物理 - 唯象学 · 物理学 2011-05-05 Mikhail Shaposhnikov , Igor Tkachev

We show that in large-field inflationary scenarios, superheavy (many orders of magnitude larger than the weak scale) dark matter will be produced in cosmologically interesting quantities if superheavy stable particles exist in the mass…

高能物理 - 唯象学 · 物理学 2016-08-25 Daniel J. H. Chung , Edward W. Kolb , Antonio Riotto

We propose a minimal extension of the standard model of particle physics to accommodate cosmic inflation, dark matter and light neutrino masses. While the inflationary phase is obtained from a modified chaotic inflation scenario, consistent…

高能物理 - 唯象学 · 物理学 2020-04-15 Debasish Borah , Dibyendu Nanda , Abhijit Kumar Saha

We propose a simple mechanism of light dark matter (DM) production from the decay of the oscillating inflaton condensation. If the reheating temperature after inflation is higher than the inflaton mass, which is of the same order of the…

高能物理 - 唯象学 · 物理学 2021-04-21 Takeo Moroi , Wen Yin

We study generation of baryon number asymmetry and both abundance of dark matter and dark energy on the basis of global symmetry and its associating flat directions in a supersymmetric model. We assume the existence of a model independent…

天体物理学 · 物理学 2009-11-13 Daijiro Suematsu

The beyond-the-standard-model scenario in this work is motivated from the observations of neutrino masses, anomalous magnetic moments of electron and muon, and dark matter in the Universe. We explain these observations by extending the…

高能物理 - 唯象学 · 物理学 2026-05-11 Vandana Sahdev

We present a string-based picture of the cosmological evolution in which (CP-violating) gravitational anomalies acting during the inflationary phase of the universe cause the vacuum energy density to "run" with the effective Hubble…

高能物理 - 理论 · 物理学 2019-07-01 Spyros Basilakos , Nick E. Mavromatos , Joan Sola

We propose a unified theory of dark matter (DM) genesis and baryogenesis. It explains the observed link between the DM density and the baryon density, and is fully testable by a combination of collider experiments and precision tests. Our…

高能物理 - 唯象学 · 物理学 2010-10-04 Lawrence J. Hall , John March-Russell , Stephen M. West

The similar cosmological energy budgets in visible baryons and dark matter motivate one to consider a common origin for the generation of both. We outline the key features of scenarios that can accommodate a unified framework for the…

高能物理 - 唯象学 · 物理学 2015-06-04 Hooman Davoudiasl , Rabindra N. Mohapatra

We study a mechanism through which the cosmic dark matter density can be explained simultaneously with the observed baryon asymmetry of the Universe. At the core of our proposal lie the out-of-equilibrium scattering processes of bath…

高能物理 - 唯象学 · 物理学 2022-09-15 Andreas Goudelis , Dimitrios Karamitros , Pantelis Papachristou , Vassilis C. Spanos

In this work, we interpret the 3-3-1-1 model when the B-L and 3-3-1 breaking scales behave simultaneously as the inflation scale. This setup not only realizes the previously-achieved consequences of inflation and leptogenesis, but also…

高能物理 - 唯象学 · 物理学 2017-04-04 D. T. Huong , P. V. Dong

We demonstrate that in a class of the $U(1)'$ extension of the Standard Model (SM), under which all the Standard Model matter fields are uncharged and the additional neutral gauge boson $Z'$ couples to a set of heavy nonstandard fermions,…

高能物理 - 唯象学 · 物理学 2018-09-12 Gautam Bhattacharyya , Maíra Dutra , Yann Mambrini , Mathias Pierre

In this paper, we investigate the common parameter space of dark matter and leptogenesis in the $U(1)_{B-L}$ symmetry. This model involves a complex scalar $\phi$, sterile neutrinos $N$, and Majorana dark matter $\chi$, where only dark…

高能物理 - 唯象学 · 物理学 2024-07-30 Ang Liu , Feng-Lan Shao , Zhi-Long Han , Yi Jin , Honglei Li

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…

天体物理学 · 物理学 2008-11-26 P. Q. Hung , Eduard Masso , Gabriel Zsembinszki

We consider the production of asymmetric dark matter during hidden sector baryogenesis. We consider a particular supersymmetric model where the dark matter candidate has a number density approximately equal to the baryon number density,…

高能物理 - 唯象学 · 物理学 2011-10-03 Bhaskar Dutta , Jason Kumar

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…

高能物理 - 唯象学 · 物理学 2019-06-26 Anirban Biswas , Sandhya Choubey , Laura Covi , Sarif Khan

Explaining baryon asymmetry, dark matter and inflation are important elements of a successful theory that extends beyond the Standard Model of particle physics. In this paper we explore these issues within the Next-to-Minimal Supersymmetric…

高能物理 - 唯象学 · 物理学 2017-04-25 Csaba Balazs , Anupam Mazumdar , Ernestas Pukartas , Graham White

We present a new mechanism for creating the observed cosmic matter-antimatter asymmetry which satisfies all three Sakharov conditions from one common thread, gravitational waves. We generate lepton number through the gravitational anomaly…

高能物理 - 理论 · 物理学 2014-03-18 Stephon H. S. Alexander , Michael E. Peskin , M. M. Sheikh-Jabbari