On the Suppression of the Dark Matter-Nucleon Scattering Cross Section in the SE₆SSM by Roman Nevzorov

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Leptogenesis and Dark Matter–Nucleon Scattering Cross Section in the SE₆SSM by Roman Nevzorov

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Searching for TeV Dark Matter in Irregular Dwarf Galaxies with HAWC Observatory by R. Alfaro, C. Alvarez, J. C. Arteaga-Velázquez, D. Avila Rojas, H. A. Ayala Solares, R. Babu, E. Belmont-Moreno, K. S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, O. Chaparro-Amaro, U. Cotti, J. Cotzomi, E. De la Fuente, R. Diaz Hernandez, B. L. Dingus, M. A. DuVernois, M. Durocher, J. C. Díaz-Vélez, C. Espinoza, K. L. Fan, N. Fraija, J. A. García-González, F. Garfias, M. M. González, J. P. Harding, S. Hernández-Cadena, D. Huang, F. Hueyotl-Zahuantitla, A. Iriarte, V. Joshi, S. Kaufmann, D. Kieda, J. Lee, H. León Vargas, J. T. Linnemann, A. L. Longinotti, G. Luis-Raya, K. Malone, O. Martinez, J. Martínez-Castro, J. A. Matthews, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, N. Omodei, Y. Pérez Araujo, E. G. Pérez-Pérez, C. D. Rho, D. Rosa-González, H. Salazar, D. Salazar-Gallegos, A. Sandoval, J. Serna-Franco, Y. Son, R. W. Springer, O. Tibolla, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, L. Villaseñor, X. Wang, E. Willox, H. Zhou, C. de León, The HAWC Collaboration, V. Gammaldi, E. Karukes, P. Salucci

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Axion-mediated Transport of Fast Radio Bursts Originating in Inner Magnetospheres of Magnetars by Anirudh Prabhu

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Barrow Holographic Dark Energy Model in Bianchi Type-III Universe with Quintessence by Chandra Rekha Mahanta, Dibyajyoti Das

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The Hough Stream Spotter: A New Method for Detecting Linear Structure in Resolved Stars and Application to the Stellar Halo of M31 by Sarah Pearson, Susan E. Clark, Alexis J. Demirjian, Kathryn V. Johnston, Melissa K. Ness, Tjitske K. Starkenburg, Benjamin F. Williams, Rodrigo A. Ibata

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Ursa Major III/UNIONS 1: The Darkest Galaxy Ever Discovered? by Raphaël Errani, Julio F. Navarro, Simon E. T. Smith, Alan W. McConnachie

Subjects: “…Cold dark matter…”
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On the Existence, Rareness, and Uniqueness of Quenched H i-rich Galaxies in the Local Universe by Xiao Li, Cheng Li, H. J. Mo, Jianhong Hu, Jing Wang, Ting Xiao

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Velocity Acoustic Oscillations on Cosmic Dawn 21 cm Power Spectrum as a Probe of Small-scale Density Fluctuations by Xin Zhang, Hengjie Lin, Meng Zhang, Bin Yue, Yan Gong, Yidong Xu, Xuelei Chen

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Can Cuspy Dark-matter-dominated Halos Hold Cored Stellar Mass Distributions? by Jorge Sánchez Almeida, Angel R. Plastino, Ignacio Trujillo

Subjects: “…Cold dark matter…”
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Structure, Kinematics, and Observability of the Large Magellanic Cloud’s Dynamical Friction Wake in Cold versus Fuzzy Dark Matter by Hayden R. Foote, Gurtina Besla, Philip Mocz, Nicolás Garavito-Camargo, Lachlan Lancaster, Martin Sparre, Emily C. Cunningham, Mark Vogelsberger, Facundo A. Gómez, Chervin F. P. Laporte

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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

“…However, the cold dark-matter model faces persistent challenges on the scales of galaxies. …”
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Electroweak loop contributions to the direct detection of wino dark matter by John Ellis, Natsumi Nagata, Keith A. Olive, Jiaming Zheng

“…Abstract Electroweak loop corrections to the matrix elements for the spin-independent scattering of cold dark matter particles on nuclei are generally small, typically below the uncertainty in the local density of cold dark matter. …”
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The effects of inelastic self-interacting dark matter on galactic halo properties v/ by Dibert, Karia Radh

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The Cusp–Core Problem in Gas-Poor Dwarf Spheroidal Galaxies by Pierre Boldrini

“…One of the most promising solutions to this cold dark matter small-scale issue is the stellar feedback, but it seems to be only designed for gas-rich dwarfs. …”
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Primordial neutrinos: hot in SM–GR–$$\Lambda $$ Λ -CDM, cold in SM–LGT by Ahmad Borzou

“…Assuming that neutrinos as heavy as 1 eV are the cold dark matter, the lower bound on the dimensionless coupling constant of LGT is derived to be $$10^{-7}$$ 10-7 which is small enough to be consistent with the upper bound that can be placed by the electroweak precision tests. …”
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Non-Relativistic Limit of Embedding Gravity as General Relativity with Dark Matter by Sergey Paston

“…Then, we construct a non-relativistic limit of these equations, in which the motion of embedding matter turns out to be slow enough so that it can play the role of cold dark matter. The non-relativistic embedding matter turns out to have a certain self-interaction, which could be useful in the context of solving the core-cusp problem that appears in the <inline-formula><math display="inline"><semantics><mi mathvariant="sans-serif">Λ</mi></semantics></math></inline-formula>-Cold Dark Matter (<inline-formula><math display="inline"><semantics><mi mathvariant="sans-serif">Λ</mi></semantics></math></inline-formula>CDM) model.…”
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Detecting the invisible universe with neutrinos and dark matter by Kaboth, Asher C. (Asher Cunningham)

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Spatial correlations in a redshift survey of apm galaxy clusters by Dalton, G, Efstathiou, G, Maddox, S, Sutherland, W

“…These results are consistent with the amplitude for ξcc expected in the standard cold dark matter model on scales ≲10 h-1 Mpc and are lower than the amplitude (r0 ∼ 25 h-1 Mpc) found by Bahcall and Soneira from the Abell catalog. …”

Non-standard structure formation scenarios by Knebe, A, Little, B, Islam, R, Devriendt, J, Mahmood, A, Silk, J

“…Observations on galactic scales seem to be in contradiction with recent high resolution N-body simulations. This so-called cold dark matter (CDM) crisis has been addressed in several ways, ranging from a change in fundamental physics by introducing self-interacting cold dark matter particles to a tuning of complex astrophysical processes such as global and/or local feedback. …”