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Supersymmetric Dark Matter

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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.
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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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Galactic Searches for Dark Matter

TL;DR: For nearly a century, more mass has been measured in galaxies than is contained in the luminous stars and gas as discussed by the authors, and it has become clear that the dark matter in galaxies is not comprised of known astronomical objects or baryonic matter.
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Atomic Dark Matter

TL;DR: In this article, the early universe formation of hydrogen-like dark atoms was studied and it was shown that weak-scale dark atoms can accommodate hyperfine splittings of order 100 keV consistent with the inelastic dark matter interpretation of the DAMA data while naturally evading direct detection bounds.
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Dark Matter Detection in the Light of Recent Experimental Results

TL;DR: In this article, a review of the dark matter in the universe is presented, with particular emphasis on Weakly Interacting Massive Particles (WIMPs) and their candidates.
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A Markov chain Monte Carlo analysis of the CMSSM

TL;DR: In this paper, a comprehensive exploration of the Constrained MSSM parameter space employing a Markov Chain Monte Carlo technique and a Bayesian analysis is performed, which includes uncertainties arising from theoretical approximations as well as from residual experimental errors of relevant Standard Model parameters.
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Microlensing constraints on primordial black holes with the Subaru/HSC Andromeda observation

TL;DR: In this paper, the authors carried out a 7 hour-long observation of the Andromeda galaxy (M31) with the Subaru Hyper Suprime-Cam to search for microlensing of stars in M31 by primordial black holes lying in the halo regions of the Milky Way (MW) and M31.
References
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The Early Universe

TL;DR: In this article, the Robertson-Walker Metric is used to measure the radius of the Planck Epoch in the expanding universe, which is a measure of the number of atoms in the universe.
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CP Violation in the Renormalizable Theory of Weak Interaction

TL;DR: In this article, it was shown that no CP-violating interactions exist in the quartet scheme without introducing any other new fields, and that the strong interaction must be chiral SU ( 4) X SU( 4) invariant as precisely as the conservation of the third component of the iso-spin.
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Partial Symmetries of Weak Interactions

TL;DR: In this paper, the weak and electromagnetic interactions of leptons are examined under the hypothesis that the weak interactions are mediated by vector bosons, and it is shown that the simplest partially-symmetric model reproducing the observed electromagnetic and weak interactions requires the existence of at least four vector-boson fields (including the photon).
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