Neutralino pair production in a $γγ$ Collider

Details Neutralino pair production in a $γγ$ Collider Neutralino pair production in a $γγ$ Collider

2003-11-06

arxiv.org/abs/hep-ph/0311076v2

Eur.Phys.J.C32:561-574,2004

Physics

High Energy Physics

High Energy Physics - Phenomenology

14 pages and 9 figures

Scientific paper

10.1140/epjc/s2003-01520-x

We present a complete 1-loop study of the process $\gamma \gamma \to \tchi^0_i \tchi^0_j$ 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 $\tchi^0_i \tchi^0_j \to \gamma\gamma$ 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.

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