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Related papers: Mesogenesis through the Ephemeral Dark Decay of Be…

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We introduce $\text{Dark}_{CP}$ Mesogenesis in which Standard Model mesons, either $B_{s,d}^0$, $B^\pm$ or $B_c^\pm$, undergo out-of-equilibrium dark CP violating decays to Standard Model and dark sector baryons. With order one CP violation…

High Energy Physics - Phenomenology · Physics 2025-10-24 Gilly Elor

Mechanisms of Mesogenesis generate the baryon asymmetry and dark matter of the Universe through late-time decays of Standard Model mesons into baryons and dark matter states. Utilizing the CP violation in the meson systems themselves, the…

High Energy Physics - Phenomenology · Physics 2026-03-31 Chaja Baruch , Gilly Elor , Jared M. Goldberg , Omer Shtaif , Yotam Soreq

We leverage the CP violation in charged $B$ meson decays to generate the observed baryon asymmetry and dark matter at $\mathcal{O}(10 \text{ MeV})$ temperatures. We realize this in two scenarios: $B_c^+$ Mesogenesis and $B^+$ Mesogenesis.…

High Energy Physics - Phenomenology · Physics 2022-04-13 Fatemeh Elahi , Gilly Elor , Robert McGehee

$B$ mesogenesis offers an interesting mechanism to generate the baryon asymmetry of the universe by converting the CP violation of the Standard Model into a net baryon number asymmetry. In this work we refine and extend the $B$ mesogenesis…

High Energy Physics - Phenomenology · Physics 2026-01-28 M. Burgos Marcos , A. Verheyden , K. K. Vos

The similar densities of dark matter and baryons in the universe imply that they might arise from the same ultraviolet model. The B-Mesogenesis, which assumes dark matter is charged under the baryon number, attempts to simultaneously…

High Energy Physics - Phenomenology · Physics 2024-08-20 Yong Zheng , Jian-Nan Ding , Dong-Hao Li , Lei-Yi Li , Cai-Dian Lü , Fu-Sheng Yu

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…

High Energy Physics - Phenomenology · Physics 2019-02-22 Gilly Elor , Miguel Escudero , Ann E. Nelson

Production of the matter-antimatter asymmetry in the $B$-Mesogenesis mechanism is directly related to the branching fraction of seemingly baryon number violating decays of $B$ mesons into a light Standard Model baryon and missing energy.…

High Energy Physics - Phenomenology · Physics 2023-03-01 Gilly Elor , Alfredo Walter Mario Guerrera

Is the Standard Model Charge-Parity (CP) violation ever enough to generate the observed baryon asymmetry? Yes! We introduce a mechanism of baryogenesis (and dark matter production) that can generate the entire observed baryon asymmetry of…

High Energy Physics - Phenomenology · Physics 2024-08-26 Gilly Elor , Rachel Houtz , Seyda Ipek , Martha Ulloa

Low-scale baryogenesis could be discovered at $B$-factories and the LHC. In the $B$-Mesogenesis paradigm [G. Elor, M. Escudero, and A. E. Nelson, PRD 99, 035031 (2019), arXiv:1810.00880], the CP violating oscillations and subsequent decays…

High Energy Physics - Phenomenology · Physics 2021-09-07 Gonzalo Alonso-Álvarez , Gilly Elor , Miguel Escudero

The $B$-Mesogenesis model explains the matter-antimatter asymmetry and leads to the right amount of dark matter in the Universe. In particular, this model predicts new decay channels of the $b$ quark. We investigate the modification of…

High Energy Physics - Phenomenology · Physics 2024-12-20 Alexander Lenz , Ali Mohamed , Zachary Wüthrich

According to the $B$-mesogenesis framework, the baryon asymmetry of the Universe and dark matter can be simultaneously generated through CP-violating $B$-meson oscillations. In this mechanism, $B$-mesons decay into a Standard Model baryon…

High Energy Physics - Phenomenology · Physics 2026-05-14 M. A. Abri , N. Hajirasouliha , K. Azizi

Low-scale baryogenesis and dark matter generation can occur via the production of neutral $B$ mesons at MeV temperatures in the early Universe, which undergo CP-violating oscillations and subsequently decay into a dark sector. In this work,…

High Energy Physics - Phenomenology · Physics 2020-04-22 Gonzalo Alonso-Álvarez , Gilly Elor , Ann E. Nelson , Huangyu Xiao

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

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…

High Energy Physics - Phenomenology · Physics 2023-10-13 Debasish Borah , Arnab Dasgupta , Matthew Knauss , Indrajit Saha

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 consider a scenario where the baryon asymmetry in the SM arises from a portal coupling to a CP-violating hidden sector, without any explicit violation of baryon or lepton number in either sector. While no net baryon number is generated,…

High Energy Physics - Phenomenology · Physics 2026-05-26 Can Kilic , Sanjay Mathai

We propose a new mechanism to simultaneously explain the observed dark matter abundance and the baryon asymmetry of the Universe. The mechanism is based on the Filtered Dark Matter scenario, where dark matter particles acquire a large mass…

High Energy Physics - Phenomenology · Physics 2022-08-24 Michael J. Baker , Moritz Breitbach , Joachim Kopp , Lukas Mittnacht , Yotam Soreq

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…

High Energy Physics - Phenomenology · Physics 2019-06-26 Anirban Biswas , Sandhya Choubey , Laura Covi , Sarif Khan

We present a testable mechanism of low-scale baryogenesis and dark matter production in which neither baryon nor lepton number are violated. Charged $D$ mesons are produced out-of-equilibrium at tens of MeV temperatures. The $D$ mesons…

High Energy Physics - Phenomenology · Physics 2021-02-12 Gilly Elor , Robert McGehee
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