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Dynamically Induced Topological Inflation

We propose an inflation model in which the inflationary era is driven by the strong dynamics of <math display="inline"><mi>S</mi><mi>p</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo>&...

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Autores principales: Choi, Gongjun, Lin, Weikang, Yanagida, Tsutomu T.
Lenguaje:eng
Publicado: 2022
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.107.036005
http://cds.cern.ch/record/2806559
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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 propose an inflation model in which the inflationary era is driven by the strong dynamics of <math display="inline"><mi>S</mi><mi>p</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></math> gauge theory. The quark condensation in the confined phase of <math display="inline"><mi>S</mi><mi>p</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></math> gauge theory generates the inflaton potential comparable to the energy of the thermal bath at the time of phase transition. Afterwards, with a super-Planckian field value at the global minimum, the inflation commences at a false vacuum region lying between true vacuum regions and hence the name “topological inflation.” Featured by the huge separation between the scale of the false vacuum (<math display="inline"><mi>V</mi><mo stretchy="false">(</mo><mn>0</mn><msup><mo stretchy="false">)</mo><mrow><mn>1</mn><mo stretchy="false">/</mo><mn>4</mn></mrow></msup><mo>∼</mo><msup><mn>10</mn><mn>15</mn></msup><mtext> </mtext><mtext> </mtext><mi>GeV</mi></math>) and the field value at the global minimum (<math display="inline"><msub><mi>ϕ</mi><mi>min</mi></msub><mo>∼</mo><msub><mi>M</mi><mi>P</mi></msub></math>), the model can be consistent with cosmic microwave background (CMB) observables without suffering from the initial condition problems. Crucially, this is achieved only with some mild tuning of parameters in <math display="inline"><mi>V</mi><mo stretchy="false">(</mo><mi>ϕ</mi><mo stretchy="false">)</mo></math>. In addition to <math display="inline"><mi>S</mi><mi>p</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></math>, this model is based on an anomaly free <math display="inline"><msub><mi>Z</mi><mrow><mn>6</mn><mi>R</mi></mrow></msub></math> discrete <math display="inline"><mi>R</mi></math> symmetry. Remarkably, while all parameters are fixed by CMB observations, the model predicts a hierarchy of energy scales including the inflation scale, supersymmetry-breaking scale, R-symmetry breaking scale, Higgsino mass and the right-handed neutrino mass given in terms of the dynamical scale of <math display="inline"><mi>S</mi><mi>p</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></math>.
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language eng
publishDate 2022
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spelling cern-28065592023-02-24T03:58:50Zdoi:10.1103/PhysRevD.107.036005http://cds.cern.ch/record/2806559engChoi, GongjunLin, WeikangYanagida, Tsutomu T.Dynamically Induced Topological InflationParticle Physics - TheoryGeneral Relativity and CosmologyAstrophysics and AstronomyParticle Physics - PhenomenologyWe propose an inflation model in which the inflationary era is driven by the strong dynamics of <math display="inline"><mi>S</mi><mi>p</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></math> gauge theory. The quark condensation in the confined phase of <math display="inline"><mi>S</mi><mi>p</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></math> gauge theory generates the inflaton potential comparable to the energy of the thermal bath at the time of phase transition. Afterwards, with a super-Planckian field value at the global minimum, the inflation commences at a false vacuum region lying between true vacuum regions and hence the name “topological inflation.” Featured by the huge separation between the scale of the false vacuum (<math display="inline"><mi>V</mi><mo stretchy="false">(</mo><mn>0</mn><msup><mo stretchy="false">)</mo><mrow><mn>1</mn><mo stretchy="false">/</mo><mn>4</mn></mrow></msup><mo>∼</mo><msup><mn>10</mn><mn>15</mn></msup><mtext> </mtext><mtext> </mtext><mi>GeV</mi></math>) and the field value at the global minimum (<math display="inline"><msub><mi>ϕ</mi><mi>min</mi></msub><mo>∼</mo><msub><mi>M</mi><mi>P</mi></msub></math>), the model can be consistent with cosmic microwave background (CMB) observables without suffering from the initial condition problems. Crucially, this is achieved only with some mild tuning of parameters in <math display="inline"><mi>V</mi><mo stretchy="false">(</mo><mi>ϕ</mi><mo stretchy="false">)</mo></math>. In addition to <math display="inline"><mi>S</mi><mi>p</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></math>, this model is based on an anomaly free <math display="inline"><msub><mi>Z</mi><mrow><mn>6</mn><mi>R</mi></mrow></msub></math> discrete <math display="inline"><mi>R</mi></math> symmetry. Remarkably, while all parameters are fixed by CMB observations, the model predicts a hierarchy of energy scales including the inflation scale, supersymmetry-breaking scale, R-symmetry breaking scale, Higgsino mass and the right-handed neutrino mass given in terms of the dynamical scale of <math display="inline"><mi>S</mi><mi>p</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></math>.We propose an inflation model in which the inflationary era is driven by the strong dynamics of $Sp(2)$ gauge theory. The quark condensation in the confined phase of $Sp(2)$ gauge theory generates the inflaton potential comparable to the energy of the thermal bath at the time of phase transition. Afterwards, with super-Planckian global minimum, the inflation commences at a false vacuum region lying between true vacuum regions and hence the name "topological inflation". Featured by the huge separation between the scale of the false vacuum ($V(0)^{1/4}\sim10^{15}{\rm GeV}$) and the global minimum ($\langle\phi\rangle\sim M_{P}$), the model can be consistent with CMB observables without suffering from the initial condition problem. Crucially, this is achieved without any fine-tuning of parameters in $V(\phi)$. In addition to $Sp(2)$, this model is based on an anomaly free $Z_{6R}$ discrete $R$ symmetry. Remarkably, while all parameters are fixed by CMB observations, the model predicts a hierarchy of energy scales including the inflation scale, SUSY-breaking scale, R-symmetry breaking scale, Higgsino mass and the right-handed neutrino mass given in terms of the dynamical scale of $Sp(2)$.arXiv:2204.03675CERN-TH-2022-061oai:cds.cern.ch:28065592022-04-07
spellingShingle Particle Physics - Theory
General Relativity and Cosmology
Astrophysics and Astronomy
Particle Physics - Phenomenology
Choi, Gongjun
Lin, Weikang
Yanagida, Tsutomu T.
Dynamically Induced Topological Inflation
title Dynamically Induced Topological Inflation
title_full Dynamically Induced Topological Inflation
title_fullStr Dynamically Induced Topological Inflation
title_full_unstemmed Dynamically Induced Topological Inflation
title_short Dynamically Induced Topological Inflation
title_sort dynamically induced topological inflation
topic Particle Physics - Theory
General Relativity and Cosmology
Astrophysics and Astronomy
Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.107.036005
http://cds.cern.ch/record/2806559
work_keys_str_mv AT choigongjun dynamicallyinducedtopologicalinflation
AT linweikang dynamicallyinducedtopologicalinflation
AT yanagidatsutomut dynamicallyinducedtopologicalinflation