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相关论文: Moduli induced cogenesis of baryon asymmetry and d…

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Late-decaying string moduli dilute the baryon asymmetry of the universe created in any previous era. The reheat temperature for such moduli is below a GeV, thus motivating baryogenesis at very low temperatures. We present an extension of…

高能物理 - 唯象学 · 物理学 2014-11-21 Rouzbeh Allahverdi , Bhaskar Dutta , Kuver Sinha

We propose a simple model in which the baryon asymmetry and dark matter are created via the decays and inverse decays of QCD-triplet scalars, at least one of which must be in the TeV mass range. Singlet fermions produced in these decays…

高能物理 - 唯象学 · 物理学 2020-07-01 Brian Shuve , David Tucker-Smith

Low-scale supersymmetry breaking in string motivated theories implies the presence of O(100) TeV scale moduli, which generically lead to a significant modification of the history of the universe prior to Big Bang Nucleosynthesis. Such an…

高能物理 - 唯象学 · 物理学 2015-05-30 Gordon Kane , Jing Shao , Scott Watson , Hai-Bo Yu

The observational relation between the density of baryon and dark matter in the Universe, $\Omega_{\rm DM}/\Omega_B\simeq 5$, is one of the most difficult problems to solve in modern cosmology. We discuss a scenario that explains this…

高能物理 - 唯象学 · 物理学 2013-05-30 Kohei Kamada , Masahide Yamaguchi

The appearance of scalar/moduli fields in the early universe, as motivated by string theory, naturally leads to non-thermal "moduli cosmology". Such cosmology provides a consistent framework where the generation of radiation, baryons, and…

高能物理 - 唯象学 · 物理学 2019-05-28 Mu-Chun Chen , Volodymyr Takhistov

We propose a novel framework where baryon asymmetry of the universe can arise due to forbidden decay of dark matter (DM) enabled by finite-temperature effects in the vicinity of a first order phase transition (FOPT). In order to implement…

高能物理 - 唯象学 · 物理学 2023-10-13 Debasish Borah , Arnab Dasgupta , Matthew Knauss , Indrajit Saha

We propose late-time moduli decay as the common origin of baryons and dark matter. The baryon asymmetry is produced from the decay of new TeV scale particles, while dark matter is created from the (chain) decay of R-parity odd particles…

高能物理 - 唯象学 · 物理学 2011-04-22 Rouzbeh Allahverdi , Bhaskar Dutta , Kuver Sinha

We present a simple extension of the standard model that gives rise to baryogenesis a has a dark matter candidate of O(GeV) mass. A minimal set of new fields required for baryogenesis includes two O(TeV) colored scalars and a singlet…

高能物理 - 唯象学 · 物理学 2013-08-09 Rouzbeh Allahverdi , Bhaskar Dutta

We propose a new mechanism where a multi-component dark sector generates the observed dark matter abundance and baryon asymmetry and thus addresses the coincidence between the two. The thermal freeze-out of dark matter annihilating into…

高能物理 - 唯象学 · 物理学 2022-03-08 Xiaoyong Chu , Yanou Cui , Josef Pradler , Michael Shamma

We explore a mechanism for producing the baryon asymmetry and dark matter in models with multiple hidden sectors that are Standard-Model-like but with varying Higgs mass parameters. If the field responsible for reheating the Standard Model…

高能物理 - 唯象学 · 物理学 2024-04-08 Hassan Easa , Thomas Gregoire , Daniel Stolarski , Catarina Cosme

We present a simple mechanism which allows the simultaneous generation of the baryon asymmetry of the Universe along with its dark matter content. To this goal, we employ the out-of-equilibrium decays of heavy bath states into a feebly…

高能物理 - 唯象学 · 物理学 2022-02-17 Andreas Goudelis , Pantelis Papachristou , Vassilis C. Spanos

In some models of supersymmetry breaking, modulus fields are heavy enough to decay before BBN. But the large entropy produced via moduli decay significantly dilutes the preexisting baryon asymmetry of the universe. We study whether…

高能物理 - 唯象学 · 物理学 2008-11-26 Masahiro Kawasaki , Kazunori Nakayama

We extend the standard model with two iso-singlet color triplet scalars, one singlet real scalar and one singlet fermion. The new fields are odd under an unbroken Z_2 discrete symmetry while the standard model particles are even. The decays…

高能物理 - 唯象学 · 物理学 2008-11-26 Pei-Hong Gu

In the context of Twin Higgs models, we study a simple mechanism that simultaneously generates asymmetries in the dark and visible sector through the out-of-equilibrium decay of a TeV scale particle charged under a combination of baryon and…

高能物理 - 唯象学 · 物理学 2016-08-24 Marco Farina , Angelo Monteux , Chang Sub Shin

We present a new mechanism of Baryogenesis and dark matter production in which both the dark matter relic abundance and the baryon asymmetry arise from neutral $B$ meson oscillations and subsequent decays. This set-up is testable at hadron…

高能物理 - 唯象学 · 物理学 2019-02-22 Gilly Elor , Miguel Escudero , Ann E. Nelson

We discuss a supersymmetric model for cogenesis of dark and baryonic matter where the dark matter (DM) has mass in the 8-10 GeV range as indicated by several direct detection searches including most recently the CDMS experiment with the…

高能物理 - 唯象学 · 物理学 2015-06-15 Rouzbeh Allahverdi , Bhaskar Dutta , Rabindra N. Mohapatra , Kuver Sinha

We study a scenario for baryogenesis in modular cosmology and discuss its implications for the moduli stabilization mechanism and the supersymmetry (SUSY) breaking scale. If moduli fields dominate the Universe and decay into the standard…

高能物理 - 唯象学 · 物理学 2015-06-18 Koji Ishiwata , Kwang Sik Jeong , Fuminobu Takahashi

The nature of dark matter (DM) particles and the mechanism that provides their measured relic abundance are currently unknown. In this paper we investigate inert scalar and vector like fermion doublet DM candidates with a charge asymmetry…

高能物理 - 唯象学 · 物理学 2015-05-30 Chiara Arina , Narendra Sahu

String/ M-theory compactifications predict the existence of a modulus field with a mass of 100-10000 TeV. Its decay at MeV-temperatures generates large amounts of entropy and washes out any previously produced baryon asymmetry. We describe…

高能物理 - 唯象学 · 物理学 2020-03-04 Gordon Kane , Martin Wolfgang Winkler

We put forward a new proposal for generating the baryon asymmetry of the universe by making use of the dynamics of a $\mathrm{U}(1)$ scalar field coupled to dark matter. High dark matter densities cause the $\mathrm{U}(1)$ symmetry to break…

高能物理 - 唯象学 · 物理学 2017-11-22 Jeremy Sakstein , Mark Trodden
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