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Related papers: B-ball Dark Matter and Baryogenesis

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Although the dark matter is usually assumed to be some form of elementary particle, primordial black holes (PBHs) could also provide some of it. However, various constraints restrict the possible mass windows to $10^{16}$ - $10^{17}\,$g,…

Cosmology and Nongalactic Astrophysics · Physics 2020-09-08 Bernard Carr , Florian Kuhnel

Minutes into the big bang, nucleosynthesis finds 96 percent of matter nonreactive. Massive pure disk protogalaxies must be formed in the early universe as their galaxies are found at high redshift. Surrounded by hot gas, they made little…

Astrophysics · Physics 2011-11-29 David E. Rosenberg

Baryogenesis during the electroweak phase transition is a plausible scenario for for the origin of matter in the Universe. Furthermore, it has the advantage over other scenarios in that one can imagine that much of the physics involved may…

High Energy Physics - Phenomenology · Physics 2016-09-01 David B. Kaplan

We present a novel baryogenesis mechanism in which the asymmetry is sourced from heavy particles which either gain their mass or are created during bubble expansion in a strong first order phase transition. These particles then decay in a…

High Energy Physics - Phenomenology · Physics 2022-01-12 Iason Baldes , Simone Blasi , Alberto Mariotti , Alexander Sevrin , Kevin Turbang

We investigate the Q-ball decay in the gauge-mediated SUSY breaking. Q balls decay mainly into nucleons, and partially into gravitinos, while they are kinematically forbidden to decay into sparticles which would be cosmologically harmful.…

High Energy Physics - Phenomenology · Physics 2015-05-28 Shinta Kasuya , Masahiro Kawasaki

A new mechanism has been proposed to simultaneously explain the presence of dark matter and the matter-antimatter asymmetry in the universe. This scenario predicts exotic $B$ meson decays into a baryon and a dark sector anti-baryon…

High Energy Physics - Experiment · Physics 2023-05-08 BABAR Collaboration , J. P. Lees , V. Poireau , V. Tisserand , E. Grauges , A. Palano , G. Eigen , D. N. Brown , Yu. G. Kolomensky , M. Fritsch , H. Koch , R. Cheaib , C. Hearty , T. S. Mattison , J. A. McKenna , R. Y. So , V. E. Blinov , A. R. Buzykaev , V. P. Druzhinin , V. B. Golubev , E. A. Kozyrev , E. A. Kravchenko , A. P. Onuchin , S. I. Serednyakov , Yu. I. Skovpen , E. P. Solodov , K. Yu. Todyshev , A. J. Lankford , B. Dey , J. W. Gary , O. Long , A. M. Eisner , W. S. Lockman , W. Panduro Vazquez , D. S. Chao , C. H. Cheng , B. Echenard , K. T. Flood , D. G. Hitlin , J. Kim , Y. Li , D. X. Lin , S. Middleton , T. S. Miyashita , P. Ongmongkolkul , J. Oyang , F. C. Porter , M. Röhrken , Z. Huard , B. T. Meadows , B. G. Pushpawela , M. D. Sokoloff , L. Sun , J. G. Smith , S. R. Wagner , D. Bernard , M. Verderi , D. Bettoni , C. Bozzi , R. Calabrese , G. Cibinetto , E. Fioravanti , I. Garzia , E. Luppi , V. Santoro , A. Calcaterra , R. de Sangro , G. Finocchiaro , S. Martellotti , P. Patteri , I. M. Peruzzi , M. Piccolo , M. Rotondo , A. Zallo , S. Passaggio , C. Patrignani , B. J. Shuve , H. M. Lacker , B. Bhuyan , U. Mallik , C. Chen , J. Cochran , S. Prell , A. V. Gritsan , N. Arnaud , M. Davier , F. Le Diberder , A. M. Lutz , G. Wormser , D. J. Lange , D. M. Wright , J. P. Coleman , E. Gabathuler , D. E. Hutchcroft , D. J. Payne , C. Touramanis , A. J. Bevan , F. Di Lodovico , R. Sacco , G. Cowan , Sw. Banerjee , D. N. Brown , C. L. Davis , A. G. Denig , W. Gradl , K. Griessinger , A. Hafner , K. R. Schubert , R. J. Barlow , G. D. Lafferty , R. Cenci , A. Jawahery , D. A. Roberts , R. Cowan , S. H. Robertson , R. M. Seddon , N. Neri , F. Palombo , L. Cremaldi , R. Godang , D. J. Summers , P. Taras , G. De Nardo , C. Sciacca , G. Raven , C. P. Jessop , J. M. LoSecco , K. Honscheid , R. Kass , A. Gaz , M. Margoni , M. Posocco , G. Simi , F. Simonetto , R. Stroili , S. Akar , E. Ben-Haim , M. Bomben , G. R. Bonneaud , G. Calderini , J. Chauveau , G. Marchiori , J. Ocariz , M. Biasini , E. Manoni , A. Rossi , G. Batignani , S. Bettarini , M. Carpinelli , G. Casarosa , M. Chrzaszcz , F. Forti , M. A. Giorgi , A. Lusiani , B. Oberhof , E. Paoloni , M. Rama , G. Rizzo , J. J. Walsh , L. Zani , A. J. S. Smith , F. Anulli , R. Faccini , F. Ferrarotto , F. Ferroni , A. Pilloni , G. Piredda , C. Bünger , S. Dittrich , O. Grünberg , M. Heß , T. Leddig , C. Voß , R. Waldi , T. Adye , F. F. Wilson , S. Emery , G. Vasseur , D. Aston , C. Cartaro , M. R. Convery , J. Dorfan , W. Dunwoodie , M. Ebert , R. C. Field , B. G. Fulsom , M. T. Graham , C. Hast , W. R. Innes , P. Kim , D. W. G. S. Leith , S. Luitz , D. B. MacFarlane , D. R. Muller , H. Neal , B. N. Ratcliff , A. Roodman , M. K. Sullivan , J. Va'vra , W. J. Wisniewski , M. V. Purohit , J. R. Wilson , A. Randle-Conde , S. J. Sekula , H. Ahmed , N. Tasneem , M. Bellis , P. R. Burchat , E. M. T. Puccio , M. S. Alam , J. A. Ernst , R. Gorodeisky , N. Guttman , D. R. Peimer , A. Soffer , S. M. Spanier , J. L. Ritchie , R. F. Schwitters , J. M. Izen , X. C. Lou , F. Bianchi , F. De Mori , A. Filippi , D. Gamba , L. Lanceri , L. Vitale , F. Martinez-Vidal , A. Oyanguren , J. Albert , A. Beaulieu , F. U. Bernlochner , G. J. King , R. Kowalewski , T. Lueck , C. Miller , I. M. Nugent , J. M. Roney , R. J. Sobie , T. J. Gershon , P. F. Harrison , T. E. Latham , R. Prepost , S. L. Wu

In this letter, we propose a novel scenario which simultaneously explains $\mathcal{O}(10)M_\odot$ primordial black holes (PBHs) and dark matter in the minimally supersymmetric standard model. Gravitational waves (GWs) events detected by…

Cosmology and Nongalactic Astrophysics · Physics 2018-08-22 Fuminori Hasegawa , Masahiro Kawasaki

What is commonly called the reheat temperature, $T_{RH}$, is not the maximum temperature obtained after inflation. The maximum temperature is, in fact, much larger than $T_{RH}$. As an application of this we consider the production of…

High Energy Physics - Phenomenology · Physics 2016-08-25 Daniel J. H. Chung , Edward W. Kolb , Antonio Riotto

Dark Matter might be an accidentally stable baryon of a new confining gauge interaction. We extend previous studies exploring the possibility that the DM is made of dark quarks heavier than the dark confinement scale. The resulting…

High Energy Physics - Phenomenology · Physics 2017-11-21 Andrea Mitridate , Michele Redi , Juri Smirnov , Alessandro Strumia

Dark matter coupled solely gravitationally can be produced through the decay of primordial black holes in the early universe. If the dark matter is lighter than the initial black hole temperature, it could be warm enough to be subject to…

Cosmology and Nongalactic Astrophysics · Physics 2020-09-23 Iason Baldes , Quentin Decant , Deanna C. Hooper , Laura Lopez-Honorez

In cold dark matter cosmology, the baryonic components of galaxies are thought to be mixed with and embedded in non-baryonic and non-relativistic dark matter, which dominates the total mass of the galaxy and its dark matter halo. In the…

We describe how difficult it is to realise baryogenesis in models where the fundamental scale in nature is as low as TeV. The problem becomes even more challenging if we assume that there are only {\it two} extra compact spatial dimensions,…

High Energy Physics - Phenomenology · Physics 2007-05-23 Anupam Mazumdar , Rouzbeh Allahverdi , Kari Enqvist , Abdel Pérez-Lorenzana

Generic axion models give rise to axion domain walls in the early Universe and they have to disappear not to overclose the universe, thus limiting the nature of discrete symmetry allowed in these type of models. Through QCD sphalerons, net…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. N. Nayak , U. A. Yajnik

We find that the Hawking radiation of black holes can create the baryon number in the Higgs phase vacuum of the extended standard model with 2-Higgs doublets. We propose new scenarios of baryogenesis based on the black holes, and one of our…

High Energy Physics - Phenomenology · Physics 2007-05-23 Yukinori Nagatani

The large discrepancy between the amount of baryons that were synthesized in Big-Bang and that we detect at $z=0$ locked in stars inside galaxies and in hot/cold gas in galaxies. goup and clusters, is a well known crucial issue for present…

Astrophysics · Physics 2015-06-24 M. Persic , P. Salucci

We propose a model for the cosmological formation of superheavy Q-Balls in the mass range $10^{-7} \, M_{\odot}$ to $10^{6} \, M_{\odot}$. The model is based on a hidden sector scalar potential motivated by broken scale invariance, for…

High Energy Physics - Phenomenology · Physics 2026-04-28 J. McDonald

We study the formation of Q-balls in the early universe, concentrating on potentials with a cubic or quartic attractive interaction. Large Q-balls can form via solitosynthesis, a process of gradual charge accretion, provided some primordial…

High Energy Physics - Phenomenology · Physics 2009-11-07 Marieke Postma

A new dark sector anti-baryon, denoted $\psi_{\text{D}}$, could be produced in decays of $B$ mesons. This letter presents a search for $B^{+} \rightarrow \psi_{\text{D}} + \text{p}$ (and the charge conjugate) decays in $e^{+}e^{-}$…

High Energy Physics - Experiment · Physics 2023-10-16 The BABAR Collaboration

We discuss baryogenesis in scenarios where the Universe is reheated to temperatures $\lesssim 100\,$GeV by the decay of long-lived massive particles into energetic SM particles. Before its thermalization, the center-of-mass energy in…

High Energy Physics - Phenomenology · Physics 2023-01-18 Joerg Jaeckel , Wen Yin

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…

High Energy Physics - Phenomenology · Physics 2022-09-15 Andreas Goudelis , Dimitrios Karamitros , Pantelis Papachristou , Vassilis C. Spanos