Leptogenesis and Dark Matter–Nucleon Scattering Cross Section in the SE<sub>6</sub>SSM

The <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>E</mi><mn>6</mn></msub></semantics></math></inline-formula>-inspired extension of the minimal supersy...

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Main Author: Roman Nevzorov
Format: Article
Language:English
Published: MDPI AG 2023-03-01
Series:Universe
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Online Access:https://www.mdpi.com/2218-1997/9/3/137
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author Roman Nevzorov
author_facet Roman Nevzorov
author_sort Roman Nevzorov
collection DOAJ
description The <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>E</mi><mn>6</mn></msub></semantics></math></inline-formula>-inspired extension of the minimal supersymmetric (SUSY) standard model (MSSM) with an extra <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>U</mi><msub><mrow><mo>(</mo><mn>1</mn><mo>)</mo></mrow><mi>N</mi></msub></mrow></semantics></math></inline-formula> gauge symmetry, under which right-handed neutrinos have zero charge, involves exotic matter beyond the MSSM to ensure anomaly cancellation. We consider the variant of this extension (SE<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>6</mn></msub></semantics></math></inline-formula>SSM) in which the cold dark matter is composed of the lightest neutral exotic fermion and gravitino. The observed baryon asymmetry can be induced in this case via the decays of the lightest right-handed neutrino/sneutrino into exotic states even for relatively low reheating temperatures <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>T</mi><mi>R</mi></msub><mo>≲</mo><msup><mn>10</mn><mrow><mn>6</mn><mo>−</mo><mn>7</mn></mrow></msup><mspace width="0.166667em"></mspace><mrow><mi>G</mi><mi>e</mi><mi>V</mi></mrow></mrow></semantics></math></inline-formula>. We argue that there are some regions of the SE<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>6</mn></msub></semantics></math></inline-formula>SSM parameter space, which are safe from all current constraints, and discuss the implications of this model for collider phenomenology.
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spelling doaj.art-c0e6ac3e1a504b65aa6822442e7e64642023-11-17T14:15:58ZengMDPI AGUniverse2218-19972023-03-019313710.3390/universe9030137Leptogenesis and Dark Matter–Nucleon Scattering Cross Section in the SE<sub>6</sub>SSMRoman Nevzorov0I.E.Tamm Theory Department, P.N. Lebedev Physical Institute of the Russian Academy of Sciences, 53 Leninskiy Prospekt, 119991 Moscow, RussiaThe <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>E</mi><mn>6</mn></msub></semantics></math></inline-formula>-inspired extension of the minimal supersymmetric (SUSY) standard model (MSSM) with an extra <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>U</mi><msub><mrow><mo>(</mo><mn>1</mn><mo>)</mo></mrow><mi>N</mi></msub></mrow></semantics></math></inline-formula> gauge symmetry, under which right-handed neutrinos have zero charge, involves exotic matter beyond the MSSM to ensure anomaly cancellation. We consider the variant of this extension (SE<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>6</mn></msub></semantics></math></inline-formula>SSM) in which the cold dark matter is composed of the lightest neutral exotic fermion and gravitino. The observed baryon asymmetry can be induced in this case via the decays of the lightest right-handed neutrino/sneutrino into exotic states even for relatively low reheating temperatures <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>T</mi><mi>R</mi></msub><mo>≲</mo><msup><mn>10</mn><mrow><mn>6</mn><mo>−</mo><mn>7</mn></mrow></msup><mspace width="0.166667em"></mspace><mrow><mi>G</mi><mi>e</mi><mi>V</mi></mrow></mrow></semantics></math></inline-formula>. We argue that there are some regions of the SE<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>6</mn></msub></semantics></math></inline-formula>SSM parameter space, which are safe from all current constraints, and discuss the implications of this model for collider phenomenology.https://www.mdpi.com/2218-1997/9/3/137unified field theories and modelsmodels beyond the standard modelsupersymmetrycold dark matterleptogenesis
spellingShingle Roman Nevzorov
Leptogenesis and Dark Matter–Nucleon Scattering Cross Section in the SE<sub>6</sub>SSM
Universe
unified field theories and models
models beyond the standard model
supersymmetry
cold dark matter
leptogenesis
title Leptogenesis and Dark Matter–Nucleon Scattering Cross Section in the SE<sub>6</sub>SSM
title_full Leptogenesis and Dark Matter–Nucleon Scattering Cross Section in the SE<sub>6</sub>SSM
title_fullStr Leptogenesis and Dark Matter–Nucleon Scattering Cross Section in the SE<sub>6</sub>SSM
title_full_unstemmed Leptogenesis and Dark Matter–Nucleon Scattering Cross Section in the SE<sub>6</sub>SSM
title_short Leptogenesis and Dark Matter–Nucleon Scattering Cross Section in the SE<sub>6</sub>SSM
title_sort leptogenesis and dark matter nucleon scattering cross section in the se sub 6 sub ssm
topic unified field theories and models
models beyond the standard model
supersymmetry
cold dark matter
leptogenesis
url https://www.mdpi.com/2218-1997/9/3/137
work_keys_str_mv AT romannevzorov leptogenesisanddarkmatternucleonscatteringcrosssectioninthesesub6subssm