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Open AccessJournal ArticleDOI

Supersymmetric Dark Matter

TLDR
In this article, the neutralino is proposed as the lightest superpartner in many supersymmetric theories, and it is shown how to calculate the cosmological abundance of neutralino and event rates for both direct and indirect detection schemes.
About
This article is published in Physics Reports.The article was published on 2000-08-01 and is currently open access. It has received 1670 citations till now. The article focuses on the topics: Lightest Supersymmetric Particle & Weakly interacting massive particles.

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Citations
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Review of mathematics, numerical factors, and corrections for dark matter experiments based on elastic nuclear recoil

TL;DR: In this article, the authors present a systematic derivation and discussion of the practical formulae needed to design and interpret direct searches for nuclear recoil events caused by hypothetical weakly interacting dark matter particles.
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Cosmology and Fundamental Physics with the Euclid Satellite

Luca Amendola, +81 more
TL;DR: Euclid is a European Space Agency medium-class mission selected for launch in 2020 within the cosmic vision 2015-2025 program as discussed by the authors, which will explore the expansion history of the universe and the evolution of cosmic structures by measuring shapes and red-shift of galaxies as well as the distribution of clusters of galaxies over a large fraction of the sky.
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PPPC 4 DM ID: a poor particle physicist cookbook for dark matter indirect detection

TL;DR: In this article, the authors provide ingredients and recipes for computing signals of TeV-scale Dark Matter annihilations and decays in the Galaxy and beyond, and provide the propagation functions for charged particles in the galaxy, for several DM distribution profiles and sets of propagation parameters.
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Dark matter search results from the CDMS II experiment.

TL;DR: The results from the completed Cryogenic Dark Matter Search (CDMS II) experiment, which searched for dark matter in the form of weakly interacting massive particles (WIMP), cannot be interpreted with confidence as evidence for WIMP interactions, but neither event can be ruled out as representing signal.
References
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Journal ArticleDOI

CBR Anisotropy in an Open Inflation, CDM Cosmogony

TL;DR: In this article, the cosmic background radiation anisotropy, produced by energy-density fluctuations generated during an early epoch of inflation, was computed in an open cosmological model based on the cold dark matter scenario.
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Can galactic halos be made of baryons

TL;DR: Several arguments are presented indicating that the apparently non-luminous matter forming massive halos of spiral galaxies is not baryonic as mentioned in this paper, and it appears that a significant fraction of the universe may be in the form of massive neutrinos, gravitinos, monopoles, etc.
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Liquid xenon as a dark matter detector. Prospects for nuclear recoil discrimination by photon timing

TL;DR: In this paper, a likelihood analysis is proposed using the time intervals between detected photons to discriminate nuclear recoil events from radioactive background in a search for hypothetical Galactic dark matter particles, showing the background rejection achievable as a function of the number of detected photons.
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Amount of antiprotons in cosmic rays due to halo neutralino annihilation

TL;DR: In this article, the antiproton-to-proton flux ratio generated by neutralino-neutralino annihilation in the galactic halo was evaluated, considering the most general compositions for the relic neutralinos and modelling the neutralino local density according to its relic abundance.
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First results from the LUX dark matter experiment at the Sanford Underground Research Facility

D. S. Akerib, +101 more