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Higgs in Space!

We consider the possibility that the Higgs can be produced in dark matter annihilations, appearing as a line in the spectrum of gamma rays at an energy determined by the masses of the WIMP and the Higgs itself. We argue that this phenomenon occurs generally in models in which the the dark sector has...

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Autores principales: Jackson, C.B., Servant, Geraldine, Shaughnessy, Gabe, Tait, Tim M.P., Taoso, Marco
Formato: info:eu-repo/semantics/article
Lenguaje:eng
Publicado: JCAP 2009
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2010/04/004
http://cds.cern.ch/record/1226309
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author Jackson, C.B.
Servant, Geraldine
Shaughnessy, Gabe
Tait, Tim M.P.
Taoso, Marco
author_facet Jackson, C.B.
Servant, Geraldine
Shaughnessy, Gabe
Tait, Tim M.P.
Taoso, Marco
author_sort Jackson, C.B.
collection CERN
description We consider the possibility that the Higgs can be produced in dark matter annihilations, appearing as a line in the spectrum of gamma rays at an energy determined by the masses of the WIMP and the Higgs itself. We argue that this phenomenon occurs generally in models in which the the dark sector has large couplings to the most massive states of the SM and provide a simple example inspired by the Randall-Sundrum vision of dark matter, whose 4d dual corresponds to electroweak symmetry-breaking by strong dynamics which respect global symmetries that guarantee a stable WIMP. The dark matter is a Dirac fermion that couples to a Z' acting as a portal to the Standard Model through its strong coupling to top quarks. Annihilation into light standard model degrees of freedom is suppressed and generates a feeble continuum spectrum of gamma rays. Loops of top quarks mediate annihilation into gamma Z, gamma h, and gamma Z', providing a forest of lines in the spectrum. Such models can be probed by the Fermi/GLAST satellite and ground-based Air Cherenkov telescopes.
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spelling cern-12263092021-05-03T20:19:03Z doi:10.1088/1475-7516/2010/04/004 http://cds.cern.ch/record/1226309 eng Jackson, C.B. Servant, Geraldine Shaughnessy, Gabe Tait, Tim M.P. Taoso, Marco Higgs in Space! Particle Physics - Phenomenology We consider the possibility that the Higgs can be produced in dark matter annihilations, appearing as a line in the spectrum of gamma rays at an energy determined by the masses of the WIMP and the Higgs itself. We argue that this phenomenon occurs generally in models in which the the dark sector has large couplings to the most massive states of the SM and provide a simple example inspired by the Randall-Sundrum vision of dark matter, whose 4d dual corresponds to electroweak symmetry-breaking by strong dynamics which respect global symmetries that guarantee a stable WIMP. The dark matter is a Dirac fermion that couples to a Z' acting as a portal to the Standard Model through its strong coupling to top quarks. Annihilation into light standard model degrees of freedom is suppressed and generates a feeble continuum spectrum of gamma rays. Loops of top quarks mediate annihilation into gamma Z, gamma h, and gamma Z', providing a forest of lines in the spectrum. Such models can be probed by the Fermi/GLAST satellite and ground-based Air Cherenkov telescopes. We consider the possibility that the Higgs can be produced in dark matter annihilations, appearing as a line in the spectrum of gamma rays at an energy determined by the masses of the WIMP and the Higgs itself. We argue that this phenomenon occurs generally in models in which the the dark sector has large couplings to the most massive states of the SM and provide a simple example inspired by the Randall-Sundrum vision of dark matter, whose 4d dual corresponds to electroweak symmetry-breaking by strong dynamics which respect global symmetries that guarantee a stable WIMP. The dark matter is a Dirac fermion that couples to a Z' acting as a portal to the Standard Model through its strong coupling to top quarks. Annihilation into light standard model degrees of freedom is suppressed and generates a feeble continuum spectrum of gamma rays. Loops of top quarks mediate annihilation into gamma Z, gamma h, and gamma Z', providing a forest of lines in the spectrum. Such models can be probed by the Fermi/GLAST satellite and ground-based Air Cherenkov telescopes. info:eu-repo/grantAgreement/EC/FP7/237920 info:eu-repo/semantics/openAccess Education Level info:eu-repo/semantics/article http://cds.cern.ch/record/1226309 JCAP JCAP, (2010) pp. 004 2009-12-02
spellingShingle Particle Physics - Phenomenology
Jackson, C.B.
Servant, Geraldine
Shaughnessy, Gabe
Tait, Tim M.P.
Taoso, Marco
Higgs in Space!
title Higgs in Space!
title_full Higgs in Space!
title_fullStr Higgs in Space!
title_full_unstemmed Higgs in Space!
title_short Higgs in Space!
title_sort higgs in space!
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1088/1475-7516/2010/04/004
http://cds.cern.ch/record/1226309
http://cds.cern.ch/record/1226309
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