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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.

Papers
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Journal ArticleDOI

Erratum to "Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei" [Astroparticle Physics 29(3) (2008) 188-204]

J. Abraham, +447 more
Journal ArticleDOI

Prospects for detection of target-dependent annual modulation in direct dark matter searches

TL;DR: In this paper, the authors examined the necessary conditions for target-dependent modulation, its observability in present-day experiments, and the extent to which putative signals could identify a dark matter-nucleus differential cross section with a non-factorizable dependence on the dark matter velocity.
Journal ArticleDOI

Unified halo-independent formalism from convex hulls for direct dark matter searches

TL;DR: Using the Fenchel-Eggleston theorem for convex hulls, this article showed that any likelihood can be maximized by either a dark matter 1-speed distribution F(v) in Earth's frame or 2-Galactic velocity distribution fgal(), consisting of a sum of delta functions.
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Operations of and Future Plans for the Pierre Auger Observatory

J. Abraham, +470 more
TL;DR: Technical reports on operations and features of the Pierre Auger Observatory, including ongoing and planned enhancements and the status of the future northern hemisphere portion of the Observatory, were presented at the 31st International Cosmic Ray Conference, Lodz, Poland, as discussed by the authors.
Journal ArticleDOI

Extended Maximum Likelihood Halo-independent Analysis of Dark Matter Direct Detection Data

TL;DR: In this article, the authors extend and correct a recently proposed maximum-likelihood halo-independent method to analyze unbinned direct dark matter detection data, instead of the recoil energy as independent variable, they use the minimum speed a dark matter particle must have to impart a given recoil energy to a nucleus.