SUSY Dark Matter and Quintessence
Stefano Profumo, Piero Ullio
Abstract
We investigate the enhancement of neutralino relic density in the context of a realistic cosmological scenario with Quintessence. The accurate relic density computation we perform allows us to be sensitive to both cases with shifts in the abundance at the percent level, and to enhancements as large as 106. We thoroughly analyze the dependence on the supersymmetric spectrum and on the mass and composition of the lightest neutralino. We point out that supersymmetric models yielding a wino or higgsino-like lightest neutralino become cosmologically appealing in the presence of Quintessence.
Create a lesson
Related papers
Virtual photon bremsstrahlung in a magnetized quark-gluon-plasma
Aritra Bandyopadhyay, Krzysztof Redlich, Chihiro Sasaki
Multiboson production at multi-TeV lepton colliders as complementary probes to rare Higgs decays
Dario Buttazzo, Keshav Chaudhary, Roberto Franceschini et al.
Deviations to cobimaximal mixing in a 3+1 neutrino scenario
Diana C. Rivera-Agudelo, S. L. Tostado
HEPTABench: A framework for portable and controlled agentic evaluations in high energy physics
Tony Menzo, Alexander Roman, George T. Fleming et al.
Cosmological Consequences of a Highly Decoupled Right-handed Neutrino
Stephen F. King, Rishav Roshan, Sudipta Show
Signature of GW from the Hidden Sector in light of the Recent LZ Event
Sujit Kumar Sahoo, Narendra Sahu, Vicky Singh Thounaojam