Simple vector WIMP dark matter

Tomohiro Abe; Mitsuru Kakizaki; Shigeki Matsumoto; Osamu Seto

Simple vector WIMP dark matter

Tomohiro Abe, Mitsuru Kakizaki, Shigeki Matsumoto, Osamu Seto^*

^*Corresponding author for this work

Department of Physics

Research output: Contribution to journal › Conference article › peer-review

1 Scopus citations

Abstract

Weakly interacting massive particle (WIMP) is well known to be a good candidate for dark matter, and it is also predicted by many new physics models beyond the standard model at the TeV scale. We found that, if the WIMP is a vector particle (spin one particle) which is associated with some gauge symmetry broken at the TeV scale, the Higgs mass is preferred to be 120 − 125 GeV, as indeed has been reported by ATLAS and CMS collaborations at the Large Hadron Collider experiment. We present a vector WIMP model based on non-linear sigma model. This model is testable and strongly constrained by experiments for direct and indirect dark matter detection.

Original language	English
Journal	Proceedings of Science
Volume	161
State	Published - 2012
Event	8th International Workshop on the Dark Side of the Universe, DSU 2012 - Buzios, Rio de Janeiro, Brazil Duration: 2012/06/10 → 2012/06/15

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title = "Simple vector WIMP dark matter",

abstract = "Weakly interacting massive particle (WIMP) is well known to be a good candidate for dark matter, and it is also predicted by many new physics models beyond the standard model at the TeV scale. We found that, if the WIMP is a vector particle (spin one particle) which is associated with some gauge symmetry broken at the TeV scale, the Higgs mass is preferred to be 120 − 125 GeV, as indeed has been reported by ATLAS and CMS collaborations at the Large Hadron Collider experiment. We present a vector WIMP model based on non-linear sigma model. This model is testable and strongly constrained by experiments for direct and indirect dark matter detection.",

author = "Tomohiro Abe and Mitsuru Kakizaki and Shigeki Matsumoto and Osamu Seto",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s).; 8th International Workshop on the Dark Side of the Universe, DSU 2012 ; Conference date: 10-06-2012 Through 15-06-2012",

year = "2012",

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T1 - Simple vector WIMP dark matter

AU - Abe, Tomohiro

AU - Kakizaki, Mitsuru

AU - Matsumoto, Shigeki

AU - Seto, Osamu

PY - 2012

Y1 - 2012

N2 - Weakly interacting massive particle (WIMP) is well known to be a good candidate for dark matter, and it is also predicted by many new physics models beyond the standard model at the TeV scale. We found that, if the WIMP is a vector particle (spin one particle) which is associated with some gauge symmetry broken at the TeV scale, the Higgs mass is preferred to be 120 − 125 GeV, as indeed has been reported by ATLAS and CMS collaborations at the Large Hadron Collider experiment. We present a vector WIMP model based on non-linear sigma model. This model is testable and strongly constrained by experiments for direct and indirect dark matter detection.

AB - Weakly interacting massive particle (WIMP) is well known to be a good candidate for dark matter, and it is also predicted by many new physics models beyond the standard model at the TeV scale. We found that, if the WIMP is a vector particle (spin one particle) which is associated with some gauge symmetry broken at the TeV scale, the Higgs mass is preferred to be 120 − 125 GeV, as indeed has been reported by ATLAS and CMS collaborations at the Large Hadron Collider experiment. We present a vector WIMP model based on non-linear sigma model. This model is testable and strongly constrained by experiments for direct and indirect dark matter detection.

UR - http://www.scopus.com/inward/record.url?scp=85052908530&partnerID=8YFLogxK

M3 - 会議記事

AN - SCOPUS:85052908530

SN - 1824-8039

VL - 161

JO - Proceedings of Science

JF - Proceedings of Science

T2 - 8th International Workshop on the Dark Side of the Universe, DSU 2012

Y2 - 10 June 2012 through 15 June 2012

ER -

Simple vector WIMP dark matter

Abstract

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