Right-handed sneutrino cosmology and hadron collider signatures

André De Gouvêa; Shrihari Gopalakrishna; Werner Porod

doi:10.1063/1.2735165

Right-handed sneutrino cosmology and hadron collider signatures

André De Gouvêa^*, Shrihari Gopalakrishna, Werner Porod

^*Corresponding author for this work

Physics and Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

It is possible that the right-handed sneutrino is the lightest supersymmetric particle (LSP). We consider the cosmological implications of such an LSP, particularly under what conditions it can lead to the observed relic density. We then discuss the Tevatron and LHC signatures of this LSP.

Original language	English (US)
Title of host publication	SUSY06
Subtitle of host publication	14th International Conference on Supersymmetry and the Unification of Fundamental Interactions
Pages	221-224
Number of pages	4
DOIs	https://doi.org/10.1063/1.2735165
State	Published - 2007
Event	SUSY06: 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions - Irvine, CA, United States Duration: Jun 12 2006 → Jun 17 2006

Publication series

Name	AIP Conference Proceedings
Volume	903
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	SUSY06: 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions
Country/Territory	United States
City	Irvine, CA
Period	6/12/06 → 6/17/06

Keywords

Hadron collider
Sneutrino
Supersymmetry

ASJC Scopus subject areas

General Physics and Astronomy

Access to Document

10.1063/1.2735165

Cite this

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title = "Right-handed sneutrino cosmology and hadron collider signatures",

abstract = "It is possible that the right-handed sneutrino is the lightest supersymmetric particle (LSP). We consider the cosmological implications of such an LSP, particularly under what conditions it can lead to the observed relic density. We then discuss the Tevatron and LHC signatures of this LSP.",

keywords = "Hadron collider, Sneutrino, Supersymmetry",

author = "{De Gouv{\^e}a}, Andr{\'e} and Shrihari Gopalakrishna and Werner Porod",

year = "2007",

doi = "10.1063/1.2735165",

language = "English (US)",

isbn = "0735404100",

series = "AIP Conference Proceedings",

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note = "SUSY06: 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions ; Conference date: 12-06-2006 Through 17-06-2006",

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De Gouvêa, A, Gopalakrishna, S & Porod, W 2007, Right-handed sneutrino cosmology and hadron collider signatures. in SUSY06: 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions. AIP Conference Proceedings, vol. 903, pp. 221-224, SUSY06: 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, Irvine, CA, United States, 6/12/06. https://doi.org/10.1063/1.2735165

Right-handed sneutrino cosmology and hadron collider signatures. / De Gouvêa, André; Gopalakrishna, Shrihari; Porod, Werner.
SUSY06: 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions. 2007. p. 221-224 (AIP Conference Proceedings; Vol. 903).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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AU - De Gouvêa, André

AU - Gopalakrishna, Shrihari

AU - Porod, Werner

PY - 2007

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N2 - It is possible that the right-handed sneutrino is the lightest supersymmetric particle (LSP). We consider the cosmological implications of such an LSP, particularly under what conditions it can lead to the observed relic density. We then discuss the Tevatron and LHC signatures of this LSP.

AB - It is possible that the right-handed sneutrino is the lightest supersymmetric particle (LSP). We consider the cosmological implications of such an LSP, particularly under what conditions it can lead to the observed relic density. We then discuss the Tevatron and LHC signatures of this LSP.

KW - Hadron collider

KW - Sneutrino

KW - Supersymmetry

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Right-handed sneutrino cosmology and hadron collider signatures

Abstract

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Keywords

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