publication . Preprint . Article . Other literature type . 2019

Baryogenesis and Dark Matter from $B$ Mesons

Elor, Gilly; Escudero, Miguel; Nelson, Ann E.;
Open Access English
  • Published: 20 Feb 2019
  • Country: Spain
Abstract
Comment: 17 pages, 6 figures. v2: references added, corrected the antinucleon abundance calculation (sec III.C.iii), and included comments on the viability of a measurement of the decay of $b$-flavored baryons into mesons and missing energy at hadron colliders (sec IV.A.iii). v3: matches the published version
Subjects
arXiv: High Energy Physics::ExperimentHigh Energy Physics::PhenomenologyNuclear TheoryNuclear ExperimentAstrophysics::Cosmology and Extragalactic Astrophysics
free text keywords: High Energy Physics - Phenomenology, Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Experiment, Physics and Astronomy (miscellaneous), B meson, Baryogenesis, Physics, Particle physics, Dark matter
Funded by
EC| ELUSIVES
Project
ELUSIVES
The Elusives Enterprise: Asymmetries of the Invisible Universe
  • Funder: European Commission (EC)
  • Project Code: 674896
  • Funding stream: H2020 | MSCA-ITN-ETN
,
EC| InvisiblesPlus
Project
InvisiblesPlus
InvisiblesPlus
  • Funder: European Commission (EC)
  • Project Code: 690575
  • Funding stream: H2020 | MSCA-RISE
,
EC| DARKHORIZONS
Project
DARKHORIZONS
Dark Matter and the Early Universe in the LHC Era
  • Funder: European Commission (EC)
  • Project Code: 648680
  • Funding stream: H2020 | ERC | ERC-COG
61 references, page 1 of 5

[1] K. Agashe and G. Servant, JCAP 0502, 002 (2005), arXiv:hep-ph/0411254 [hep-ph].

[2] P. A. R. Ade et al. (Planck), Astron. Astrophys. 594, A13 (2016), arXiv:1502.01589 [astro-ph.CO].

[3] N. Aghanim et al. (Planck), (2018), arXiv:1807.06209 [astro-ph.CO].

[4] R. H. Cyburt, B. D. Fields, K. A. Olive, and T.-H. Yeh, Rev. Mod. Phys. 88, 015004 (2016), arXiv:1505.01076 [astro-ph.CO].

[5] M. Tanabashi et al. (ParticleDataGroup), Phys. Rev. D98, 030001 (2018).

[6] A. D. Sakharov, Pisma Zh. Eksp. Teor. Fiz. 5, 32 (1967), [Usp. Fiz. Nauk161,61(1991)].

[7] S. Nussinov, Phys. Lett. 165B, 55 (1985).

[8] S. Dodelson and L. M. Widrow, Phys. Rev. D42, 326 (1990).

[9] S. M. Barr, R. S. Chivukula, and E. Farhi, Phys. Lett. B241, 387 (1990).

[10] D. B. Kaplan, Phys. Rev. Lett. 68, 741 (1992).

[11] G. R. Farrar and G. Zaharijas, Phys. Rev. Lett. 96, 041302 (2006), arXiv:hep-ph/0510079 [hep-ph].

[12] D. E. Kaplan, M. A. Luty, and K. M. Zurek, Phys. Rev. D79, 115016 (2009), arXiv:0901.4117 [hep-ph].

[13] Y. Grossman, Y. Nir, and R. Rattazzi, Adv. Ser. Direct. High Energy Phys. 15, 755 (1998), [,755(1997)], arXiv:hep-ph/9701231 [hep-ph].

[14] H. Davoudiasl, D. E. Morrissey, K. Sigurdson, and S. Tulin, Phys. Rev. Lett. 105, 211304 (2010), arXiv:1008.2399 [hep-ph].

[15] M. Artuso, G. Borissov, and A. Lenz, Rev. Mod. Phys. 88, 045002 (2016), arXiv:1511.09466 [hep-ph].

61 references, page 1 of 5
Abstract
Comment: 17 pages, 6 figures. v2: references added, corrected the antinucleon abundance calculation (sec III.C.iii), and included comments on the viability of a measurement of the decay of $b$-flavored baryons into mesons and missing energy at hadron colliders (sec IV.A.iii). v3: matches the published version
Subjects
arXiv: High Energy Physics::ExperimentHigh Energy Physics::PhenomenologyNuclear TheoryNuclear ExperimentAstrophysics::Cosmology and Extragalactic Astrophysics
free text keywords: High Energy Physics - Phenomenology, Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Experiment, Physics and Astronomy (miscellaneous), B meson, Baryogenesis, Physics, Particle physics, Dark matter
Funded by
EC| ELUSIVES
Project
ELUSIVES
The Elusives Enterprise: Asymmetries of the Invisible Universe
  • Funder: European Commission (EC)
  • Project Code: 674896
  • Funding stream: H2020 | MSCA-ITN-ETN
,
EC| InvisiblesPlus
Project
InvisiblesPlus
InvisiblesPlus
  • Funder: European Commission (EC)
  • Project Code: 690575
  • Funding stream: H2020 | MSCA-RISE
,
EC| DARKHORIZONS
Project
DARKHORIZONS
Dark Matter and the Early Universe in the LHC Era
  • Funder: European Commission (EC)
  • Project Code: 648680
  • Funding stream: H2020 | ERC | ERC-COG
61 references, page 1 of 5

[1] K. Agashe and G. Servant, JCAP 0502, 002 (2005), arXiv:hep-ph/0411254 [hep-ph].

[2] P. A. R. Ade et al. (Planck), Astron. Astrophys. 594, A13 (2016), arXiv:1502.01589 [astro-ph.CO].

[3] N. Aghanim et al. (Planck), (2018), arXiv:1807.06209 [astro-ph.CO].

[4] R. H. Cyburt, B. D. Fields, K. A. Olive, and T.-H. Yeh, Rev. Mod. Phys. 88, 015004 (2016), arXiv:1505.01076 [astro-ph.CO].

[5] M. Tanabashi et al. (ParticleDataGroup), Phys. Rev. D98, 030001 (2018).

[6] A. D. Sakharov, Pisma Zh. Eksp. Teor. Fiz. 5, 32 (1967), [Usp. Fiz. Nauk161,61(1991)].

[7] S. Nussinov, Phys. Lett. 165B, 55 (1985).

[8] S. Dodelson and L. M. Widrow, Phys. Rev. D42, 326 (1990).

[9] S. M. Barr, R. S. Chivukula, and E. Farhi, Phys. Lett. B241, 387 (1990).

[10] D. B. Kaplan, Phys. Rev. Lett. 68, 741 (1992).

[11] G. R. Farrar and G. Zaharijas, Phys. Rev. Lett. 96, 041302 (2006), arXiv:hep-ph/0510079 [hep-ph].

[12] D. E. Kaplan, M. A. Luty, and K. M. Zurek, Phys. Rev. D79, 115016 (2009), arXiv:0901.4117 [hep-ph].

[13] Y. Grossman, Y. Nir, and R. Rattazzi, Adv. Ser. Direct. High Energy Phys. 15, 755 (1998), [,755(1997)], arXiv:hep-ph/9701231 [hep-ph].

[14] H. Davoudiasl, D. E. Morrissey, K. Sigurdson, and S. Tulin, Phys. Rev. Lett. 105, 211304 (2010), arXiv:1008.2399 [hep-ph].

[15] M. Artuso, G. Borissov, and A. Lenz, Rev. Mod. Phys. 88, 045002 (2016), arXiv:1511.09466 [hep-ph].

61 references, page 1 of 5
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