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19952022
most citedThe effects of He I 10830 on helium abundance determinations

413 citations · 4.4k across the 66 of their papers we have counts for

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Showing 2006Show all

13 papers · 1 filter

hep-ph2006

Searching for Dark Matter in Unification Models: A Hint from Indirect Sensitivities towards Future Signals in Direct Detection and B-decay

Keith A. Olive

A comparison is made between accelerator and direct detection constraints in constrained versions of the minimal supersymmetric standard model. Models considered are based on mSUGR…

astro-ph2006182 cited

Coupled Variations of Fundamental Couplings and Primordial Nucleosynthesis

Alain Coc, Nelson J. Nunes, Keith A. Olive +2

The effect of variations of the fundamental nuclear parameters on big-bang nucleosynthesis are modeled and discussed in detail taking into account the interrelations between the fu…

astro-ph2006152 cited

Bound-State Effects on Light-Element Abundances in Gravitino Dark Matter Scenarios

Richard H. Cyburt, John Ellis, Brian D. Fields +2

If the gravitino is the lightest supersymmetric particle and the long-lived next-to-lightest sparticle (NSP) is the stau, the charged partner of the tau lepton, it may be metastabl…

hep-ph200637 cited

The Fate of SUSY Flat Directions and their Role in Reheating

Keith A. Olive, Marco Peloso

We consider the role of supersymmetric flat directions in reheating the Universe after inflation. One or more flat directions can develop large vevs during inflation, which can pot…

hep-ph200637 cited

What if supersymmetry breaking appears below the GUT scale?

John Ellis, Keith A. Olive, Pearl Sandick

We consider the possibility that the soft supersymmetry-breaking parameters m_{1/2} and m_0 of the MSSM are universal at some scale M_{in} below the supersymmetric grand unificatio…

astro-ph200646 cited

Population III Generated Cosmic Rays and the Production of Li6

Emmanuel Rollinde, Elisabeth Vangioni, Keith A. Olive

We calculate the evolution of Li6 generated from cosmic rays produced by an early population of massive stars. The computation is performed in the framework of hierarchical structu…