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Graciela B. Gelmini

Researcher at University of California, Los Angeles

Publications -  249
Citations -  14586

Graciela B. Gelmini is an academic researcher from University of California, Los Angeles. The author has contributed to research in topics: Dark matter & Neutrino. The author has an hindex of 52, co-authored 239 publications receiving 13465 citations. Previous affiliations of Graciela B. Gelmini include University of Chicago & International Centre for Theoretical Physics.

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Direct detection of light anapole and magnetic dipole DM

TL;DR: In this paper, the authors compare direct detection data for light WIMPs with an anapole moment interaction (ADM) and a magnetic dipole moment interactions (MDM), both assuming the Standard Halo Model (SHM) for the dark halo of our galaxy and in a halo-independent manner.
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Low reheating temperatures in monomial and binomial inflationary models

TL;DR: In this article, the authors investigated the allowed range of reheating temperature values in light of the Planck 2015 results and the recent joint analysis of Cosmic Microwave Background (CMB) data from the BICEP2/Keck Array and Planck experiments, using monomial and binomial inflationary potentials.
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The exposure of the hybrid detector of the Pierre Auger Observatory

P. Abreu, +482 more
TL;DR: In this article, the authors describe the determination of the hybrid exposure for events observed by the fluorescence telescopes in coincidence with at least one water-Cherenkov detector of the surface array.
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MeV sterile neutrinos in low reheating temperature cosmological scenarios

TL;DR: In this paper, it was shown that the cosmological and astrophysical bounds on the mixings of sterile neutrinos are much less stringent than those obtained from laboratory measurements.
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What is the cosmion

TL;DR: The solar neutrino problem can be solved if the sun has accreted a sufficient number of weakly interacting particles from the dark matter of the galaxy as discussed by the authors, and three explicit particle physics models for these cosmions are given, each having a different mechanism for suppressing cosmion annihilations in the sun.