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Neutralino pair production in a $\gamma \gamma $ collider
Authors:G?J?Gounaris  J?Layssac  P?I?Porfyriadis  Email author" target="_blank">F?M?RenardEmail author
Institution:(1) Department of Theoretical Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece;(2) Physique Mathématique et Théorique, UMR 5825, Université Montpellier II, 34095 Montpellier Cedex 5, France
Abstract:We present a complete one-loop study of the process $\gamma \gamma \to {\tilde \chi}^0_i {\tilde \chi}^0_j$ and the predicted cross section in a $\gamma \gamma $ Linear Collider. A suitable numerical code, PLATONlc, valid for any set of real MSSM parameters, is released. This study and code are complementary to those suitable for dark matter detection through the inverse process ${\tilde \chi}^0_i {\tilde \chi}^0_j \to \gamma\gamma$ describing neutralino-neutralino annihilation at rest, which were presented previously. If SUSY is realized in nature, both codes should be very helpful in future astrophysical and collider studies of the neutralino sector.Received: 6 November 2003, Published online: 9 January 2004Programme drsquoActions Intégrées Franco-Hellenique, Platon 04100 UM.
Keywords:
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