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Discrete R-symmetry, various energy scales, and gravitational waves
We present a supersymmetric model where energy scales of a discrete <math display="inline"><mi>R</mi></math>-symmetry breaking (<math display="inline"><msub><mi>Z</mi><mrow><mn>6</mn><mi>R</mi></mrow...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
2022
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Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.105.055033 http://cds.cern.ch/record/2799344 |
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author | Choi, Gongjun Lin, Weikang Yanagida, Tsutomu T. |
author_facet | Choi, Gongjun Lin, Weikang Yanagida, Tsutomu T. |
author_sort | Choi, Gongjun |
collection | CERN |
description | We present a supersymmetric model where energy scales of a discrete <math display="inline"><mi>R</mi></math>-symmetry breaking (<math display="inline"><msub><mi>Z</mi><mrow><mn>6</mn><mi>R</mi></mrow></msub></math>) and cosmic inflation are commonly attributed to the confinement scale of a hidden <math display="inline"><mi>S</mi><mi>p</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></math> strong dynamics. Apart from these, the supersymmetry-breaking scale, the Higgsino mass, and the right-handed neutrino masses are all shown to stem from the <math display="inline"><msub><mi>Z</mi><mrow><mn>6</mn><mi>R</mi></mrow></msub></math> breaking scale inferred from cosmic microwave background observables. We will show that the model is characterized by the supersymmetry-breaking soft mass <math display="inline"><msub><mi>m</mi><mrow><mi>soft</mi></mrow></msub><mo>≃</mo><mn>100</mn><mi>–</mi><mn>1000</mn><mtext> </mtext><mtext> </mtext><mi>TeV</mi></math> and the reheating temperature <math display="inline"><mrow><msub><mrow><mi>T</mi></mrow><mrow><mi>rh</mi></mrow></msub><mo>≃</mo><msup><mrow><mn>10</mn></mrow><mrow><mn>9</mn></mrow></msup><mtext> </mtext><mtext> </mtext><mi>GeV</mi></mrow></math>. Then we discuss how these predictions of the model can be tested with the help of the spectrum of the gravitational wave induced by the short-lived cosmic string present during the reheating era. |
id | cern-2799344 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2022 |
record_format | invenio |
spelling | cern-27993442023-01-31T10:52:57Zdoi:10.1103/PhysRevD.105.055033http://cds.cern.ch/record/2799344engChoi, GongjunLin, WeikangYanagida, Tsutomu T.Discrete R-symmetry, various energy scales, and gravitational waveshep-thParticle Physics - Theoryastro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyWe present a supersymmetric model where energy scales of a discrete <math display="inline"><mi>R</mi></math>-symmetry breaking (<math display="inline"><msub><mi>Z</mi><mrow><mn>6</mn><mi>R</mi></mrow></msub></math>) and cosmic inflation are commonly attributed to the confinement scale of a hidden <math display="inline"><mi>S</mi><mi>p</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></math> strong dynamics. Apart from these, the supersymmetry-breaking scale, the Higgsino mass, and the right-handed neutrino masses are all shown to stem from the <math display="inline"><msub><mi>Z</mi><mrow><mn>6</mn><mi>R</mi></mrow></msub></math> breaking scale inferred from cosmic microwave background observables. We will show that the model is characterized by the supersymmetry-breaking soft mass <math display="inline"><msub><mi>m</mi><mrow><mi>soft</mi></mrow></msub><mo>≃</mo><mn>100</mn><mi>–</mi><mn>1000</mn><mtext> </mtext><mtext> </mtext><mi>TeV</mi></math> and the reheating temperature <math display="inline"><mrow><msub><mrow><mi>T</mi></mrow><mrow><mi>rh</mi></mrow></msub><mo>≃</mo><msup><mrow><mn>10</mn></mrow><mrow><mn>9</mn></mrow></msup><mtext> </mtext><mtext> </mtext><mi>GeV</mi></mrow></math>. Then we discuss how these predictions of the model can be tested with the help of the spectrum of the gravitational wave induced by the short-lived cosmic string present during the reheating era.We present a supersymmetric model where energy scales of a discrete $R$-symmetry breaking ($Z_{6R}$) and cosmic inflation are commonly attributed to the confinement scale of a hidden $Sp(2)$ strong dynamics. Apart from these, SUSY-breaking scale, the Higgsino mass and the right-handed neutrino masses are all shown to stem from $Z_{6R}$ breaking scale inferred from CMB observables. We will show that the model is characterized by the SUSY-breaking soft mass $m_{\rm soft}\simeq100-1000{\rm TeV}$ and the reheating temperature $T_{\rm rh}\simeq10^{9}{\rm GeV}$. Then we discuss how these predictions of the model can be tested with the help of the spectrum of the gravitational wave induced by the short-lived cosmic string present during the reheating era.arXiv:2201.03083CERN-TH-2022-002oai:cds.cern.ch:27993442022-01-09 |
spellingShingle | hep-th Particle Physics - Theory astro-ph.CO Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology Choi, Gongjun Lin, Weikang Yanagida, Tsutomu T. Discrete R-symmetry, various energy scales, and gravitational waves |
title | Discrete R-symmetry, various energy scales, and gravitational waves |
title_full | Discrete R-symmetry, various energy scales, and gravitational waves |
title_fullStr | Discrete R-symmetry, various energy scales, and gravitational waves |
title_full_unstemmed | Discrete R-symmetry, various energy scales, and gravitational waves |
title_short | Discrete R-symmetry, various energy scales, and gravitational waves |
title_sort | discrete r-symmetry, various energy scales, and gravitational waves |
topic | hep-th Particle Physics - Theory astro-ph.CO Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1103/PhysRevD.105.055033 http://cds.cern.ch/record/2799344 |
work_keys_str_mv | AT choigongjun discretersymmetryvariousenergyscalesandgravitationalwaves AT linweikang discretersymmetryvariousenergyscalesandgravitationalwaves AT yanagidatsutomut discretersymmetryvariousenergyscalesandgravitationalwaves |