Colloquium: Annual modulation of dark matter

By K. Freese, M. Lisanti, C. Savage. 2013

266 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/65ae2f87dc6e1a37a3eb6f2449dfdc80084ca167

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In Astronomy and Astrophysics

In Nuclear and High Energy Physics

Citations in the corpus

Form factors for dark matter capture by the Sun in effective theories (2015, methodology): “Finally, we assume the so-called standard halo model [46], with a Maxwell-Boltzmann speed distribution for f(u), and a local standard of rest velocity of 220 km s−1.”
Lectures on Dark Matter Physics (2016, background): “found in articles such as [70,72,86], but we will focus primarily on an illustrative explanation here.”
Revealing the dark matter halo with axion direct detection (2017, result): “This can be contrasted to the case in WIMP direct-detection experiments, where substructure is expected to play an important role in annual modulation studies but not necessarily have a significant impact on the total rate [86,94,100].”
Search for New Physics with Atoms and Molecules (2017, background): “Further, in the galactic rest frame the velocity distribution of DM objects is isotropic and quasi-Maxwellian, with dispersion v ≈ 290 km/s and a cutoff above the galactic escape velocity of vesc ≈ 550 km/s (Freese et al., 2013).”
Dark matter direct-detection experiments (2015, background): “As the amplitude of the variation is expected to be small, the temporal variation of the differential event rate can be written, following [108], as”
WIMP dark matter candidates and searches—current status and future prospects (2017, background): “In some cases one looks for the annual modulation of the signal due to the Earth’s movement with respect to the DM halo [153] (for review see [154]).”