Invisible and semi-invisible decays of bottom baryons
The similar densities of dark matter and baryons in the universe imply that they may arise from the same ultraviolet model. B -Mesogenesis, which assumes dark matter is charged under the baryon number, attempts to simultaneously explain the origin of baryon asymmetry and dark matter in the universe....
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| Published in | Chinese physics C Vol. 48; no. 8; p. 83109 |
|---|---|
| Main Authors | , , , , , |
| Format | Journal Article |
| Language | English |
| Published |
01.08.2024
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| Online Access | Get full text |
| ISSN | 1674-1137 2058-6132 2058-6132 |
| DOI | 10.1088/1674-1137/ad4afa |
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| Abstract | The similar densities of dark matter and baryons in the universe imply that they may arise from the same ultraviolet model.
B
-Mesogenesis, which assumes dark matter is charged under the baryon number, attempts to simultaneously explain the origin of baryon asymmetry and dark matter in the universe. In particular,
B
-Mesogenesis may induce bottom-baryon decays into invisible or semi-invisible final states, which provide a distinctive signal for probing this scenario. In this work, we systematically study the invisible decays of bottom baryons into dark matter and the semi-invisible decays of bottom baryons into a meson or a photon together with a dark matter particle. In particular, the fully invisible decay can reveal the stable particles in
B
-Mesogenesis. Some QCD-based frameworks are used to calculate the hadronic matrix elements under the
B
-Mesogenesis model. We estimate the constraints on the Wilson coefficients or the product of some new physics couplings with the Wilson coefficients according to the semi-invisible and invisible decays of bottom baryons detectable at future colliders. |
|---|---|
| AbstractList | The similar densities of dark matter and baryons in the universe imply that they may arise from the same ultraviolet model.
B
-Mesogenesis, which assumes dark matter is charged under the baryon number, attempts to simultaneously explain the origin of baryon asymmetry and dark matter in the universe. In particular,
B
-Mesogenesis may induce bottom-baryon decays into invisible or semi-invisible final states, which provide a distinctive signal for probing this scenario. In this work, we systematically study the invisible decays of bottom baryons into dark matter and the semi-invisible decays of bottom baryons into a meson or a photon together with a dark matter particle. In particular, the fully invisible decay can reveal the stable particles in
B
-Mesogenesis. Some QCD-based frameworks are used to calculate the hadronic matrix elements under the
B
-Mesogenesis model. We estimate the constraints on the Wilson coefficients or the product of some new physics couplings with the Wilson coefficients according to the semi-invisible and invisible decays of bottom baryons detectable at future colliders. |
| Author | Ding 丁, Jian-Nan 剑南 Li 李, Lei-Yi 磊毅 Lü 吕, Cai-Dian 才典 Yu 于, Fu-Sheng 福升 Zheng 郑, Yong 勇 Li 李, Dong-Hao 东浩 |
| Author_xml | – sequence: 1 givenname: Yong 勇 surname: Zheng 郑 fullname: Zheng 郑, Yong 勇 – sequence: 2 givenname: Jian-Nan 剑南 surname: Ding 丁 fullname: Ding 丁, Jian-Nan 剑南 – sequence: 3 givenname: Dong-Hao 东浩 surname: Li 李 fullname: Li 李, Dong-Hao 东浩 – sequence: 4 givenname: Lei-Yi 磊毅 surname: Li 李 fullname: Li 李, Lei-Yi 磊毅 – sequence: 5 givenname: Cai-Dian 才典 surname: Lü 吕 fullname: Lü 吕, Cai-Dian 才典 – sequence: 6 givenname: Fu-Sheng 福升 surname: Yu 于 fullname: Yu 于, Fu-Sheng 福升 |
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| Snippet | The similar densities of dark matter and baryons in the universe imply that they may arise from the same ultraviolet model.
B
-Mesogenesis, which assumes dark... |
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