Multilepton dark matter signals by J. A. Aguilar-Saavedra, J. A. Casas, J. Quilis, R. Ruiz de Austri

“…Abstract The signatures of dark matter at the LHC commonly involve, in simplified scenarios, the production of a single particle plus large missing energy, from the undetected dark matter. …”
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Dark matter and global symmetries by Yann Mambrini, Stefano Profumo, Farinaldo S. Queiroz

“…Assuming that (i) global symmetries are broken at the Planck scale, that (ii) the non-renormalizable operators mediating dark matter decay have O(1) couplings, that (iii) the dark matter is a singlet field, and that (iv) the dark matter density distribution is well described by a NFW profile, we are able to rule out fermionic, vector, and scalar dark matter candidates across a broad mass range (keV–TeV), including the WIMP regime.…”
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Gravitation, cosmology and dark matter by Mississippi Valenzuela

Subjects: “…Curvature Tensor, field equations, Friedmann equations, dark matter candidates.…”
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Rare species of dark matter by Maxim Pospelov

“…I also discuss the de-excitations on nuclear isomers through a recoil on dark matter, as well as in-situ formation of the DM-nucleus bound states.…”
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Digging for biosynthetic dark matter by Jia Jia Zhang, Bradley S Moore

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Dark Matter and Mirror World by Rabindra N. Mohapatra

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Dark matter in astrophysics/cosmology by Anne M. Green

“…These lecture notes aim to provide an introduction to dark matter from the perspective of astrophysics/cosmology. …”
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Inelastic Dirac dark matter by Anastasiia Filimonova, Sam Junius, Laura Lopez Honorez, Susanne Westhoff

Subjects: “…Dark Matter at Colliders…”
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Sterile neutrinos as dark matter by Mikhail Shaposhnikov

“…I describe the sterile neutrino dark matter candidate and discuss how it may fit into the overall picture of physics beyond the Standard Model.…”
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Simplified Dark Matter Models by Enrico Morgante

“…I review the construction of simplified models for dark matter searches. After discussing the philosophy and some simple examples, I turn the attention to the aspect of the theoretical consistency and to the implications of the necessary extensions of these models.…”
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Dark Matters on the Scale of Galaxies by Ivan de Martino, Sankha S. Chakrabarty, Valentina Cesare, Arianna Gallo, Luisa Ostorero, Antonaldo Diaferio

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Super-resonant dark matter by Csaba Csáki, Andrew Gomes, Yonit Hochberg, Eric Kuflik, Kevin Langhoff, Hitoshi Murayama

Subjects: “…Models for Dark Matter…”
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Stringballs and Planckballs for dark matter by Zhongyou Mo, Tibério de Paula Netto, Nicolò Burzillà, Leonardo Modesto

Subjects: “…Models for Dark Matter…”
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Blowing in the dark matter wind by Hannah Day, Da Liu, Markus A. Luty, Yue Zhao

Subjects: “…Models for Dark Matter…”
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Not-so-inelastic Dark Matter by Giovani Dalla Valle Garcia, Felix Kahlhoefer, Maksym Ovchynnikov, Thomas Schwetz

Subjects: “…Models for Dark Matter…”
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Enabling forbidden dark matter by Cline, James M., Liu, Hongwan, Slatyer, Tracy Robyn, Xue, Wei

“…The thermal relic density of dark matter is conventionally set by two-body annihilations. …”
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Decaying dark matter and reionization by Jubas, Jay M.

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Accidentally Asymmetric Dark Matter by Asadi, Pouya, Kramer, Eric David, Kuflik, Eric, Ridgway, Gregory W, Slatyer, Tracy R, Smirnov, Juri

“…The surviving abundance is determined by the local accidental asymmetry in each pocket. The correct dark matter abundance is obtained for $\mathcal{O}(1-100)$ PeV dark quarks, above the usual unitarity bound.…”
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Thermal squeezeout of dark matter by Asadi, Pouya, Kramer, Eric David, Kuflik, Eric, Ridgway, Gregory W, Slatyer, Tracy R, Smirnov, Juri

“…We find that during this phase transition the quarks are trapped inside contracting pockets of the deconfined phase and are compressed enough to interact at a significant rate, giving rise to a second stage of annihilation that can dramatically change the resulting dark matter abundance. As a result, the dark matter can be heavier than the often-quoted unitarity bound of $\sim100~$TeV. …”
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Semi-annihilation of dark matter by D'Eramo, Francesco, Thaler, Jesse

“…We show that the thermal relic abundance of dark matter can be affected by a new type of reaction: semi-annihilation. …”
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