2015
DOI: 10.1016/j.physrep.2014.10.002
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Abstract: a b s t r a c tIncreasingly stringent limits from LHC searches for new physics, coupled with lack of convincing signals of weakly interacting massive particle (WIMP) in dark matter searches, have tightly constrained many realizations of the standard paradigm of thermally produced WIMPs as cold dark matter. In this article, we review more generally both thermally and non-thermally produced dark matter (DM). One may classify DM models into two broad categories: one involving bosonic coherent motion (BCM) and the… Show more

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Cited by 324 publications
(332 citation statements)
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References 912 publications
(1,458 reference statements)
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“…In particular, we use the constraints obtained in Table I of [31], which gives 95% CL upper bounds on this quantity for different assumptions of the DM profile and gamma-ray energy bin. 1 In comparing to our theoretical prediction for 1 Table I by a value of approximately 2.8 (for an NFW profile). This has been confirmed with the authors of [31].…”
Section: Indirect Detectionmentioning
confidence: 65%
See 1 more Smart Citation
“…In particular, we use the constraints obtained in Table I of [31], which gives 95% CL upper bounds on this quantity for different assumptions of the DM profile and gamma-ray energy bin. 1 In comparing to our theoretical prediction for 1 Table I by a value of approximately 2.8 (for an NFW profile). This has been confirmed with the authors of [31].…”
Section: Indirect Detectionmentioning
confidence: 65%
“…WIMPs can naturally account for the observed DM abundance in the framework of standard thermal freeze-out, and they are often within reach of current and future experiments (see Ref. [1][2][3] for extensive overviews on particle DM).…”
Section: Introductionmentioning
confidence: 99%
“…While radiation is produced directly from the decay of φ, DM can be produced in several different ways [13]. For simplicity, we assume that DM is produced only from radiation by scatterings and set f m = 0.…”
mentioning
confidence: 99%
“…We do not explicitly calculate the relic abundance, but several mechanisms for the non-thermal productions have been proposed so far. For instance, it is known that the decays of long-lived heavy particles, such as gravitino, saxion and moduli field, can significantly produce the LSP after the LSP is frozen out from the thermal bath [57][58][59][60].…”
Section: Jhep08(2017)072mentioning
confidence: 99%