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We study the impact on electroweak baryogenesis from a swifter cosmological expansion induced by dark matter. We detail the experimental bounds that one can place on models that realize it, and we investigate the modifications of these…

高能物理 - 唯象学 · 物理学 2016-12-01 Marek Lewicki , Tanja Rindler-Daller , James D. Wells

In this Letter, we propose a new possible connection between dark matter relic density and baryon asymmetry of the universe. The portal between standard model sector and dark matter not only controls the relic density and detections of dark…

高能物理 - 唯象学 · 物理学 2015-05-30 Talal Ahmed Chowdhury , Miha Nemevsek , Goran Senjanovic , Yue Zhang

A new cosmological scenario is proposed in which a light scalaron of $f (R)$ gravity plays the role of dark matter. In this scenario, the scalaron initially resides at the minimum of its effective potential while the electroweak symmetry is…

高能物理 - 唯象学 · 物理学 2021-07-02 Yuri Shtanov

The extension of the standard model by a real gauge singlet scalar is the simplest but the most studied model with sometimes controversial ideas on the ability of the model to address the dark matter and the electroweak phase transition…

高能物理 - 唯象学 · 物理学 2019-07-08 Karim Ghorbani , Parsa Hossein Ghorbani

We discuss the dynamics and phenomenology of an oscillating scalar field coupled to the Higgs boson that accounts for the dark matter in the Universe. The model assumes an underlying scale invariance such that the scalar field only acquires…

高能物理 - 唯象学 · 物理学 2018-05-25 Catarina Cosme , João G. Rosa , O. Bertolami

We introduce an oscillating scalar field coupled to the Higgs that can account for all dark matter in the Universe. Due to an underlying scale invariance of this model, the dark scalar only acquires mass after the electroweak phase…

高能物理 - 唯象学 · 物理学 2019-12-02 Catarina Cosme

The nature of the cosmological dark matter remains elusive. Recent studies have advocated the possibility that dark matter could be composed of ultra-light, self-interacting bosons, forming a Bose-Einstein condensate in the very early…

宇宙学与河外天体物理 · 物理学 2014-04-22 Tanja Rindler-Daller , Paul R. Shapiro

In an earlier paper I proposed a highly symmetric semi-classical initial condition to describe the universe in the period leading up to the electroweak transition and completely determine all cosmology after that. Nothing beyond the…

宇宙学与河外天体物理 · 物理学 2022-03-25 Daniel Friedan

We show that the present dark matter abundance can be accounted for by an oscillating scalar field that acquires both mass and a non-zero expectation value from interactions with the Higgs field. The dark matter scalar field can be…

高能物理 - 唯象学 · 物理学 2018-05-03 Catarina Cosme , João G. Rosa , O. Bertolami

Beyond the Standard Model physics is required to explain both dark matter and the baryon asymmetry of the universe, the latter possibly generated during a strong first-order electroweak phase transition. While many proposed models tackle…

高能物理 - 唯象学 · 物理学 2022-10-17 Simone Biondini , Philipp Schicho , Tuomas V. I. Tenkanen

The observed dark energy in the universe might give particles inertial mass. We investigate one realization of this idea, that the dark energy field might be a decayed scalar component of a supermultiplet field in the early universe that…

天体物理学 · 物理学 2007-05-23 Robert J. Nemiroff , Bijunath Patla

Motivated by the possibility to explain dark matter abundance and strong electroweak phase transition, we consider simple extensions of the Standard Model containing singlet fields coupled with the Standard Model via a scalar portal.…

高能物理 - 唯象学 · 物理学 2015-07-15 Tommi Alanne , Kimmo Tuominen , Ville Vaskonen

The nature of dark matter and of dark energy which constitute more than $95\%$ of the energy in the Universe remains a great and unresolved question in cosmology. Cold dark matter can be made of an ultralight scalar field dominated by its…

宇宙学与河外天体物理 · 物理学 2020-12-09 J. -F. Coupechoux , A. Arbey

In this work we present a model of dark matter based on scalar-tensor theory of gravity. With this scalar field dark matter model we study the non-linear evolution of the large scale structures in the universe. The equations that govern the…

宇宙学与河外天体物理 · 物理学 2015-06-03 Mario A. Rodriguez-Meza

We consider the cosmological dynamics of a scalar field in a potential with multiple troughs and peaks. We show that the dynamics of the scalar field will evolve from light dark matter-like behaviour (such as that of a light axion) to a…

宇宙学与河外天体物理 · 物理学 2018-07-04 Takeshi Kobayashi , Pedro G. Ferreira

We study static configurations of dark matter coupled to a scalar field responsible for the dark energy of the Universe. The dark matter is modelled as a Fermi gas within the Thomas-Fermi approximation. The mass of the dark matter particles…

天体物理学 · 物理学 2009-11-13 N. Brouzakis , N. Tetradis

We discuss the possibility that dark matter corresponds to an oscillating scalar field coupled to the Higgs boson. We argue that the initial field amplitude should generically be of the order of the Hubble parameter during inflation, as a…

高能物理 - 唯象学 · 物理学 2016-06-22 Orfeu Bertolami , Catarina Cosme , João G. Rosa

The dark sector of the Universe need not be completely separable into distinct dark matter and dark energy components. We consider a model of early dark energy in which the dark energy mimics a dark matter component in both evolution and…

宇宙学与河外天体物理 · 物理学 2014-09-05 Jannis Bielefeld , Robert R. Caldwell , Eric V. Linder

We investigate the electroweak phase transition patterns for a recently proposed baryogenesis model with CP violation originated in the dark sector. The model includes a complex scalar singlet-Higgs boson portal, a $U(1)_l$ gauge lepton…

高能物理 - 唯象学 · 物理学 2023-03-22 Marcela Carena , Ying-Ying Li , Tong Ou , Yikun Wang

Recent data from cosmic ray experiments may be explained by a new GeV scale of physics. In addition the fine-tuning of supersymmetric models may be alleviated by new O(GeV) states into which the Higgs boson could decay. The presence of…

高能物理 - 唯象学 · 物理学 2011-09-27 Subinoy Das , Patrick J. Fox , Abhishek Kumar , Neal Weiner
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