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Open AccessJournal ArticleDOI

Particle Dark Matter: Evidence, Candidates and Constraints

TLDR
The current status of particle dark matter, including experimental evidence and theoretical motivations, including direct and indirect detection techniques, is discussed in this article. But the authors focus on neutralinos in models of supersymmetry and Kaluza-Klein dark matter in universal extra dimensions.
Abstract
In this review article, we discuss the current status of particle dark matter, including experimental evidence and theoretical motivations. We discuss a wide array of candidates for particle dark matter, but focus on neutralinos in models of supersymmetry and Kaluza-Klein dark matter in models of universal extra dimensions. We devote much of our attention to direct and indirect detection techniques, the constraints placed by these experiments and the reach of future experimental efforts.

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Citations
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Journal ArticleDOI

Nonperturbative effect on dark matter annihilation and gamma ray signature from the galactic center

TL;DR: In this paper, the authors evaluate the gamma ray flux in the case that the dark matter has an electroweak SU(2)_L charge in the minimal supersymmetric standard model (MSSM) when the lightest SUSY particle is the Higgsino- or Wino-like neutralino.
Journal ArticleDOI

Earth-mass dark-matter haloes as the first structures in the early Universe.

TL;DR: Supercomputer simulations of the concordance cosmological model, which assumes neutralino dark matter (at present the preferred candidate), are reported, and it is found that the first objects to form are numerous Earth-mass dark-matter haloes about as large as the Solar System.
Journal ArticleDOI

Weakly interacting massive particle-nucleus elastic scattering response

TL;DR: In this paper, a model independent formulation of WIMP-nucleon scattering was recently developed in Galilean invariant effective field theory and embedded in the nucleus, determining the most general WIMPs-Nucleus elastic response.
Journal ArticleDOI

Constraints on the Galactic Halo Dark Matter from Fermi-LAT Diffuse Measurements

Markus Ackermann, +140 more
TL;DR: In the absence of a robust dark-matter signal, constraints are presented in this paper that the dark matter signal does not exceed the observed diffuse gamma-ray emission, and the resulting limits impact the range of particle masses over which dark matter thermal production in the early Universe is possible, and challenge the interpretation of the PAMELA/Fermi-LAT cosmic ray anomalies as annihilation of dark matter.
Journal ArticleDOI

Cusps in CDM halos

TL;DR: In this paper, the inner region of a massive cluster forming in a cosmological CDM simulation with a mass resolution of 2 × 10 6 M⊙ and before z = 4.4 even 3 × 10 5 M ⊙ was resolved.
References
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Journal ArticleDOI

Cosmological parameters from SDSS and WMAP

Max Tegmark, +70 more
- 01 Jan 2004 - 
TL;DR: In this paper, the authors measured cosmological parameters using the three-dimensional power spectrum P(k) from over 200,000 galaxies in the Sloan Digital Sky Survey (SDSS) in combination with WMAP and other data.
Book

Supersymmetry and Supergravity

TL;DR: The second edition of this book appeared in 1983 and was based on a series of lectures given at Princeton in 1983 by Julius Wess as discussed by the authors, where the authors presented a general supersymmetric gauge invariant theory of chiral fields interacting with supergravity.
Book

Radiative processes in astrophysics

TL;DR: Inverse square law for a uniformly bright sphere as discussed by the authors is used to define specific intensity and its moments, which is defined as the specific intensity or brightness of a sphere in terms of specific intensity.
Book ChapterDOI

A Supersymmetry Primer

TL;DR: In this article, the authors provide a pedagogical introduction to supersymmetry, focusing on readers who are familiar with the Standard Model and quantum field theory, but who have had little or no prior exposure to superymmetry.
Book

High Energy Astrophysics

TL;DR: In this article, the authors introduce high energy astrophysics in the context of galaxies and the origin of cosmic rays in our galaxy, as well as the acceleration of high energy particles in magnetic fields.
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