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19952011
most citedHadronic Uncertainties in the Elastic Scattering of Supersymmetric Dark Matter

370 citations · 2.9k across the 46 of their papers we have counts for

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Showing 2004 · astro-phShow all

8 papers · 2 filters

astro-ph200410 cited

APS Neutrino Study: Report of the Neutrino Astrophysics and Cosmology Working Group

Steve W. Barwick, John F. Beacom, Vince Cianciolo +11

In 2002, Ray Davis and Masatoshi Koshiba were awarded the Nobel Prize in Physics ``for pioneering contributions to astrophysics, in particular for the detection of cosmic neutrinos…

astro-ph2004

Cosmological Cosmic Rays and the observed Li6 plateau in metal poor halo stars

Emmanuel Rollinde, Elisabeth Vangioni-Flam, Keith A. Olive

Very recent observations of the Li6 isotope in halo stars reveal a Li6 plateau about 1000 times above the predicted BBN abundance. We calculate the evolution of Li6 versus redshift…

astro-ph2004

Implications of a new temperature scale for halo dwarfs on LiBeB and chemical evolution

Brian D. Fields, Keith A. Olive, Elisabeth Vangioni-Flam

Big bang nucleosynthesis (BBN) and the cosmic baryon density from cosmic microwave background anisotropies together predict a primordial Li7 abundance a factor of 2--3 higher than…

astro-ph2004

New BBN limits on Physics Beyond the Standard Model from He4

Richard H. Cyburt, Brian D. Fields, Keith A. Olive +1

A recent analysis of the He4 abundance determined from observations of extragalactic HII regions indicates a significantly greater uncertainty for the He4 mass fraction. The derive…

astro-ph2004

Quintessence Models and the Cosmological Evolution of alpha

Seokcheon Lee, Keith A. Olive, Maxim Pospelov

The cosmological evolution of a quintessence-like scalar field, phi, coupled to matter and gauge fields leads to effective modifications of the coupling constants and particle mass…

astro-ph2004

A Realistic Determination of the Error on the Primordial Helium Abundance: Steps Toward Non-Parametric Nebular Helium Abundances

Keith A. Olive, Evan D. Skillman

Currently there are two significantly different observational determinations of the primordial helium abundance, and, if only statistical errors in He4 abundance determinations are…