Rescuing leptogenesis parameter space of inverse seesaw

被引：0

作者：

Mukherjee, Ananya ^{[1
]}

Saha, Abhijit Kumar ^{[2
]}

机构：

[1] Saha Inst Nucl Phys, Theory Div, 1-AF Bidhannagar, Kolkata 700064, India

[2] Inst Phys, Sainik Sch, Bhubaneswar 751005, Orissa, India

来源：

PHYSICS LETTERS B | 2024年 / 849卷

关键词：

NEUTRINO-MASS; BARYOGENESIS; SEARCH; DIRAC;

D O I：

10.1016/j.physletb.2024.138474

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In a pure inverse seesaw framework, achieving a substantial lepton asymmetry that can be converted into the observed baryon asymmetry of the Universe is extremely challenging. The difficulty arises primarily due to two reasons, (i) partial cancellation of the lepton asymmetries associated with the components of a pseudo-Dirac pair, and (ii) strong wash out caused by the inverse decays. In this work we offer two possible resolutions to overcome the above mentioned challenges considering a (3,3) ISS framework. Our first proposal is based on the assumption of a non -standard cosmological era in the pre-BBN epoch, that triggers a faster expansion of the Universe, thereby reducing the washout by several orders of magnitude. The second proposition is an alternative of first which considers a quasi-degenerate mass spectrum for the singlet heavy neutrinos, resulting into a larger order of lepton asymmetry that survives the impact of strong washout to account for the observed BAU. The viable parameters space, as obtained can be tested at present and future Lepton Flavour Violation experiments e.g. MEG and MEG II.

引用

页数：12

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