Resonant leptogenesis in minimal U(1)X extensions of the Standard Model

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Physics Letters B Pub Date : 2025-05-01 Epub Date: 2025-03-17 DOI:10.1016/j.physletb.2025.139395
Arindam Das , Yuta Orikasa
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Abstract

We investigate a general U(1)X scenario where we introduce three generations of Standard Model (SM) singlet Right Handed Neutrinos (RHNs) to generate the light neutrino mass through the seesaw mechanism after the breaking of U(1)X and electroweak symmetries. In addition to that, a general U(1)X scenario involves an SM-singlet scalar field and due to the U(1)X symmetry breaking the mass of a neutral beyond the SM (BSM) gauge boson Z is evolved. The RHNs, charged under the U(1)X scenario, can explain the origin of observed baryon asymmetry through the resonant leptogenesis process. Applying observed neutrino oscillation data we study Z and BSM scalar-induced processes to reproduce the observed baryon asymmetry. Hence we estimate bounds on the U(1)X gauge coupling (gX) and the mass of the Z (MZ) for different U(1)X charges and benchmark masses of the RHN and SM-singlet scalar. Finally, we compare our results with limits obtained from the existing limits from LEP-II and LHC. We find that depending on the U(1)X charges, the masses of RHNs and SM-singlet scalar resonant leptogenesis could provide a stronger limit on gX for MZ>5.8 TeV which could be probed by high energy scattering experiment in future.
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标准模型的最小U(1)X扩展中的共振纤生
我们研究了一个一般的U(1)X场景,我们引入了三代标准模型(SM)单重态右手中微子(RHNs),在U(1)X和电弱对称性被打破后,通过跷跷板机制产生轻中微子质量。除此之外,一般的U(1)X场景涉及SM-单重态标量场,并且由于U(1)X对称性破缺,中性粒子的质量超过SM (BSM)规范玻色子Z '被演化。在U(1)X情景下带电的rhn可以通过共振轻生过程解释观测到的重子不对称的起源。利用观测到的中微子振荡数据,我们研究了Z '和BSM的标量诱导过程,以再现观测到的重子不对称性。因此,我们估计了不同U(1)X电荷的U(1)X规范耦合(gX)和Z ‘的质量(MZ ’)的边界以及RHN和sm -单重态标量的基准质量。最后,我们将我们的结果与LEP-II和LHC的现有极限进行了比较。我们发现,根据U(1)X电荷的不同,rhn和sm -单重态标量共振轻生的质量可以在MZ ' >;5.8 TeV下提供更强的gX极限,这可以在未来的高能散射实验中进行探测。
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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