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There exists a class of cosmic strings that turn matter into antimatter (Alice strings). In a GUT where the unbroken gauge group contains charge conjugation ($C$), such strings form when a phase transition renders $C$ a discrete symmetry.…

High Energy Physics - Phenomenology · Physics 2016-09-01 Shahar Ben-Menahem , Adrian R. Cooper

We present a model of spontaneous (or dynamical) C and CP violation where it is possible to generate domains of matter and antimatter separated by cosmologically large distances. Such C(CP) violation existed only in the early universe and…

Cosmology and Nongalactic Astrophysics · Physics 2015-10-15 A. D. Dolgov , S. I. Godunov , A. S. Rudenko , I. I. Tkachev

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…

High Energy Physics - Phenomenology · Physics 2024-04-08 Hassan Easa , Thomas Gregoire , Daniel Stolarski , Catarina Cosme

In standard models of baryogenesis and of dark matter, the mechanisms which generate the densities in both sectors are unrelated to each other. In this paper we explore models which generate the baryon asymmetry through the dark matter…

High Energy Physics - Phenomenology · Physics 2010-12-24 Jessie Shelton , Kathryn M. Zurek

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…

High Energy Physics - Phenomenology · Physics 2022-02-17 Andreas Goudelis , Pantelis Papachristou , Vassilis C. Spanos

A novel mechanism for explaining the matter-antimatter asymmetry of the universe is considered. We assume that the universe starts from completely symmetric state and then, as it cools down, it undergoes a quantum-phase transition which in…

Cosmology and Nongalactic Astrophysics · Physics 2011-05-31 V. R. Shaginyan , G. S. Japaridze , M. Ya. Amusia , A. Z. Msezane , K. G. Popov

We show that both the baryon asymmetry of the Universe and the dark matter abundance can be explained within a single framework that makes use of maximally helical hypermagnetic fields produced during pseudoscalar inflation and the chiral…

High Energy Physics - Phenomenology · Physics 2019-10-10 Yann Cado , Eray Sabancilar

We propose a novel mechanism for electroweak baryogenesis in which collapsing domain walls formed by an axion-like field replace the bubble walls in a strong first-order electroweak phase transition. The axion-like particle coupling to the…

High Energy Physics - Phenomenology · Physics 2026-05-01 Yang Bai , Kun-Feng Lyu , Yue Zhao

We consider a dark matter (DM) model offering a very natural explanation of the observed relation, $\Omega_{\rm dark} \sim \Omega_{\rm visible}$. This generic consequence of the model is a result of the common origin of both types of matter…

High Energy Physics - Phenomenology · Physics 2017-09-20 Shuailiang Ge , Xunyu Liang , Ariel Zhitnitsky

The Universe may contain sufficiently small size matter-antimatter domains at temperatures of a few hundred MeV, without violating the success of Big Bang Nucleosynthesis. We demonstrate that this possibility enhances the keV scale sterile…

High Energy Physics - Phenomenology · Physics 2023-09-26 Mikhail Shaposhnikov , Alexei Yu Smirnov

The electroweak baryogenesis is studied in the charge transport mechanism with the vector-like quark model. Introducing an extra vector-like up-type quark and a singlet Higgs scalar with the mass of the order of a few hundred GeV, the…

High Energy Physics - Phenomenology · Physics 2009-10-28 Tomoko Uesugi , Akio Sugamoto , Azusa Yamaguchi

It was recently suggested that dark matter consists of ~GeV particles that carry baryon number and mix with the neutron. We demonstrate that this could allow for resonant dark matter-neutron oscillations in the early universe, at finite…

High Energy Physics - Phenomenology · Physics 2019-07-10 Torsten Bringmann , James M. Cline , Jonathan M. Cornell

The similarity of the visible and dark matter abundances indicates that they may originate via the same mechanism. If both the dark and the visible matter are charged under a generalized baryon number which remains always conserved, then…

High Energy Physics - Phenomenology · Physics 2011-12-09 Nicole F. Bell , Kalliopi Petraki , Ian M. Shoemaker , Raymond R. Volkas

We introduce a novel mechanism where the kinetic energy of a rotating axion can be dissipated by the interactions with dark magnetic monopoles. This mechanism leads to a framework where the QCD axion and dark monopoles account for the dark…

High Energy Physics - Phenomenology · Physics 2025-11-14 Raymond T. Co , Keisuke Harigaya , Isaac R. Wang , Huangyu Xiao

The comparable abundances of dark matter and baryons imply a deep connection between the dark sector and the QCD sector. In models of asymmetric dark matter, the number densities of both sectors are ensured to be similar. However, a…

High Energy Physics - Phenomenology · Physics 2025-12-09 Yi Chung

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

We propose a new scenario of baryogenesis, in which annihilation of axion domain walls generates a sizable baryon asymmetry. Successful baryogenesis is possible for a wide range of the axion mass and decay constant, $m \simeq 10^8 -10^{13}$…

High Energy Physics - Phenomenology · Physics 2015-08-13 Ryuji Daido , Naoya Kitajima , Fuminobu Takahashi

The existence of macroscopic regions with antibaryon excess in the baryon asymmetric Universe with general baryon excess is the possible consequence of practically all models of baryosynthesis. Diffusion of matter and antimatter to the…

Astrophysics · Physics 2011-05-23 M. Yu. Khlopov , R. V. Konoplich , R. Mignani , S. G. Rubin , A. S. Sakharov

We propose an alternative mechanism of baryogenesis in which a scalar baryon undergoes a percolating first-order phase transition in the early Universe. The potential barrier that divides the phases contains explicit B and CP violation and…

High Energy Physics - Phenomenology · Physics 2015-06-05 Clifford Cheung , Alex Dahlen , Gilly Elor

We find that QCD can create the cosmological matter abundance via out-of-equilibrium processes during the QCD phase transition, that is what we call the QCD preheating, where the dynamic transition of the QCD vacuum characterized by the…

High Energy Physics - Phenomenology · Physics 2023-07-17 Xin-Ru Wang , Jin-Yang Li , Seishi Enomoto , Hiroyuki Ishida , Shinya Matsuzaki