Unraveling the Scotogenic model at muon collider

Jiao Liu (School of Physics and Technology, University of Jinan, Jinan, Shandong, 250022, China; Guangxi Key Laboratory of Nuclear Physics and Nuclear Technology, Guangxi Normal University, Guilin, Guangxi, 541004, China) ; Zhi-Long Han (School of Physics and Technology, University of Jinan, Jinan, Shandong, 250022, China) ; Yi Jin (School of Physics and Technology, University of Jinan, Jinan, Shandong, 250022, China; Guangxi Key Laboratory of Nuclear Physics and Nuclear Technology, Guangxi Normal University, Guilin, Guangxi, 541004, China) ; Honglei Li (School of Physics and Technology, University of Jinan, Jinan, Shandong, 250022, China)

The Scotogenic model extends the standard model with three singlet fermion N i and one inert doublet scalar η to address the common origin of tiny neutrino mass and dark matter. For fermion dark matter N 1, a hierarchical Yukawa structure y 1 e y 1 μ y 1 τ O 1 $$ \mid {y}_{1e}\mid \ll \mid {y}_{1\mu}\mid \sim \mid {y}_{1\tau}\mid \sim \mathcal{O}(1) $$ is usually favored to satisfy constraints from lepton flavor violation and relic density. Such large μ-related Yukawa coupling would greatly enhance the pair production of charged scalar η ± at the muon collider. In this paper, we investigate the dilepton and mono-photon signature of the Scotogenic model at a 14 TeV muon collider. For the dimuon signature , we find that most viable samples can be probed with 200 fb −1 data. The ditau signature is usually less promising, but it is important to probe the small |y 1μ | region. The mono-photon signature could also probe the compressed mass region M 1 ≲ M η ± $$ {M}_{\eta^{\pm }} $$ . Masses of charged scalar η ± and dark matter N 1 can be further extracted by a binned likelihood fit of the dilepton energy.

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      "surname": "Han", 
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      "source": "Springer", 
      "value": "The Scotogenic model extends the standard model with three singlet fermion N  i  and one inert doublet scalar \u03b7 to address the common origin of tiny neutrino mass and dark matter. For fermion dark matter N 1, a hierarchical Yukawa structure   <math> <mo>\u2223</mo> <msub> <mi>y</mi> <mrow> <mn>1</mn> <mi>e</mi> </mrow> </msub> <mo>\u2223</mo> <mo>\u226a</mo> <mo>\u2223</mo> <msub> <mi>y</mi> <mrow> <mn>1</mn> <mi>\u03bc</mi> </mrow> </msub> <mo>\u2223</mo> <mo>\u223c</mo> <mo>\u2223</mo> <msub> <mi>y</mi> <mrow> <mn>1</mn> <mi>\u03c4</mi> </mrow> </msub> <mo>\u2223</mo> <mo>\u223c</mo> <mi>O</mi> <mfenced> <mn>1</mn> </mfenced> </math>  $$ \\mid {y}_{1e}\\mid \\ll \\mid {y}_{1\\mu}\\mid \\sim \\mid {y}_{1\\tau}\\mid \\sim \\mathcal{O}(1) $$  is usually favored to satisfy constraints from lepton flavor violation and relic density. Such large \u03bc-related Yukawa coupling would greatly enhance the pair production of charged scalar \u03b7  \u00b1  at the muon collider. In this paper, we investigate the dilepton and mono-photon signature of the Scotogenic model at a 14 TeV muon collider. For the dimuon signature   , we find that most viable samples can be probed with 200 fb \u22121 data. The ditau signature    is usually less promising, but it is important to probe the small |y 1\u03bc  | region. The mono-photon signature    could also probe the compressed mass region M 1 \u2272   <math> <msub> <mi>M</mi> <msup> <mi>\u03b7</mi> <mo>\u00b1</mo> </msup> </msub> </math>  $$ {M}_{\\eta^{\\pm }} $$ . Masses of charged scalar \u03b7  \u00b1  and dark matter N 1 can be further extracted by a binned likelihood fit of the dilepton energy."
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Published on:
12 December 2022
Publisher:
Springer
Published in:
Journal of High Energy Physics , Volume 2022 (2022)
Issue 12
Pages 1-34
DOI:
https://doi.org/10.1007/JHEP12(2022)057
arXiv:
2207.07382
Copyrights:
The Author(s)
Licence:
CC-BY-4.0

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