{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,1,14]],"date-time":"2026-01-14T15:32:56Z","timestamp":1768404776639,"version":"3.49.0"},"reference-count":213,"publisher":"MDPI AG","issue":"10","license":[{"start":{"date-parts":[[2021,10,15]],"date-time":"2021-10-15T00:00:00Z","timestamp":1634256000000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Symmetry"],"abstract":"<jats:p>Possible dark matter candidates in particle physics span a mass range extending over fifty orders of magnitude. In this review, we consider the range of masses from a few keV to a few hundred TeV, which is relevant for cold particle dark matter. We will consider models where dark matter arises as weakly coupled elementary fields and models where dark matter is a composite state bound by a new strong interaction. Different production mechanisms for dark matter in these models will be described. The landscape of direct and indirect searches for dark matter and some of the resulting constraints on models will be briefly discussed.<\/jats:p>","DOI":"10.3390\/sym13101945","type":"journal-article","created":{"date-parts":[[2021,10,17]],"date-time":"2021-10-17T23:25:15Z","timestamp":1634513115000},"page":"1945","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":5,"title":["Cold Particle Dark Matter"],"prefix":"10.3390","volume":"13","author":[{"ORCID":"https:\/\/orcid.org\/0000-0003-4077-6893","authenticated-orcid":false,"given":"Kimmo","family":"Tuominen","sequence":"first","affiliation":[{"name":"Department of Physics, University of Helsinki, P.O. 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Phys."},{"key":"ref_4","doi-asserted-by":"crossref","first-page":"0059","DOI":"10.1038\/s41550-017-0059","article-title":"How Dark Matter Came to Matter","volume":"1","author":"Bertone","year":"2017","journal-title":"Nat. Astron."},{"key":"ref_5","doi-asserted-by":"crossref","first-page":"023506","DOI":"10.1103\/PhysRevD.62.023506","article-title":"MeV scale reheating temperature and thermalization of neutrino background","volume":"62","author":"Kawasaki","year":"2000","journal-title":"Phys. Rev. D"},{"key":"ref_6","doi-asserted-by":"crossref","first-page":"043506","DOI":"10.1103\/PhysRevD.70.043506","article-title":"What is the lowest possible reheating temperature?","volume":"70","author":"Hannestad","year":"2004","journal-title":"Phys. Rev. D"},{"key":"ref_7","doi-asserted-by":"crossref","first-page":"043522","DOI":"10.1103\/PhysRevD.72.043522","article-title":"The Oscillation effects on thermalization of the neutrinos in the Universe with low reheating temperature","volume":"72","author":"Ichikawa","year":"2005","journal-title":"Phys. Rev. D"},{"key":"ref_8","doi-asserted-by":"crossref","first-page":"192","DOI":"10.1016\/j.astropartphys.2008.09.005","article-title":"New constraints on the reheating temperature of the universe after WMAP-5","volume":"30","author":"Pagano","year":"2008","journal-title":"Astropart. Phys."},{"key":"ref_9","doi-asserted-by":"crossref","first-page":"043541","DOI":"10.1103\/PhysRevD.95.043541","article-title":"Ultralight scalars as cosmological dark matter","volume":"95","author":"Hui","year":"2017","journal-title":"Phys. Rev. D"},{"key":"ref_10","doi-asserted-by":"crossref","first-page":"355","DOI":"10.1146\/annurev-nucl-050520-125911","article-title":"Primordial Black Holes as Dark Matter: Recent Developments","volume":"70","author":"Carr","year":"2020","journal-title":"Ann. Rev. Nucl. Part. Sci."},{"key":"ref_11","doi-asserted-by":"crossref","first-page":"365","DOI":"10.1086\/161130","article-title":"A Modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis","volume":"270","author":"Milgrom","year":"1983","journal-title":"Astrophys. J."},{"key":"ref_12","doi-asserted-by":"crossref","first-page":"083509","DOI":"10.1103\/PhysRevD.70.083509","article-title":"Relativistic gravitation theory for the MOND paradigm","volume":"70","author":"Bekenstein","year":"2004","journal-title":"Phys. Rev. D"},{"key":"ref_13","doi-asserted-by":"crossref","first-page":"011301","DOI":"10.1103\/PhysRevLett.96.011301","article-title":"Large Scale Structure in Bekenstein\u2019s theory of relativistic Modified Newtonian Dynamics","volume":"96","author":"Skordis","year":"2006","journal-title":"Phys. Rev. Lett."},{"key":"ref_14","doi-asserted-by":"crossref","first-page":"104015","DOI":"10.1103\/PhysRevD.81.104015","article-title":"Vector field models of modified gravity and the dark sector","volume":"81","author":"Zuntz","year":"2010","journal-title":"Phys. Rev. D"},{"key":"ref_15","doi-asserted-by":"crossref","first-page":"083009","DOI":"10.1103\/PhysRevD.100.083009","article-title":"Testing Dark Matter and Modifications to Gravity using Local Milky Way Observables","volume":"100","author":"Lisanti","year":"2019","journal-title":"Phys. Rev. D"},{"key":"ref_16","doi-asserted-by":"crossref","first-page":"203","DOI":"10.1140\/epjc\/s10052-018-5662-y","article-title":"The waning of the WIMP? A review of models, searches, and constraints","volume":"78","author":"Arcadi","year":"2018","journal-title":"Eur. Phys. J. C"},{"key":"ref_17","doi-asserted-by":"crossref","first-page":"1730023","DOI":"10.1142\/S0217751X1730023X","article-title":"The Dawn of FIMP Dark Matter: A Review of Models and Constraints","volume":"32","author":"Bernal","year":"2017","journal-title":"Int. J. Mod. Phys. A"},{"key":"ref_18","doi-asserted-by":"crossref","first-page":"55","DOI":"10.1016\/0370-2693(85)90689-6","article-title":"Technocosmology: Could a technibaryon excess provide a \u2018natural\u2019 missing mass candidate?","volume":"165","author":"Nussinov","year":"1985","journal-title":"Phys. Lett. B"},{"key":"ref_19","doi-asserted-by":"crossref","first-page":"1643004","DOI":"10.1142\/S0217751X16430041","article-title":"Review of strongly-coupled composite dark matter models and lattice simulations","volume":"31","author":"Kribs","year":"2016","journal-title":"Int. J. Mod. Phys. A"},{"key":"ref_20","doi-asserted-by":"crossref","first-page":"095040","DOI":"10.1103\/PhysRevD.97.095040","article-title":"Hidden strongly interacting massive particles","volume":"97","author":"Heikinheimo","year":"2018","journal-title":"Phys. Rev. D"},{"key":"ref_21","doi-asserted-by":"crossref","first-page":"191","DOI":"10.1016\/j.physletb.2015.06.080","article-title":"Minimal Asymmetric Dark Matter","volume":"748","author":"Boucenna","year":"2015","journal-title":"Phys. Lett. B"},{"key":"ref_22","doi-asserted-by":"crossref","first-page":"1","DOI":"10.1016\/j.physletb.2012.08.020","article-title":"Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC","volume":"716","author":"Aad","year":"2012","journal-title":"Phys. Lett. B"},{"key":"ref_23","doi-asserted-by":"crossref","first-page":"30","DOI":"10.1016\/j.physletb.2012.08.021","article-title":"Observation of a New Boson at a Mass of 125 GeV with the CMS Experiment at the LHC","volume":"716","author":"Chatrchyan","year":"2012","journal-title":"Phys. Lett. B"},{"key":"ref_24","doi-asserted-by":"crossref","first-page":"596","DOI":"10.1086\/381970","article-title":"Weak lensing mass reconstruction of the interacting cluster 1E0657-558: Direct evidence for the existence of dark matter","volume":"604","author":"Clowe","year":"2004","journal-title":"Astrophys. J."},{"key":"ref_25","doi-asserted-by":"crossref","first-page":"050","DOI":"10.1088\/1475-7516\/2015\/04\/050","article-title":"How rare is the Bullet Cluster (in a \u039bCDM universe)?","volume":"04","author":"Kraljic","year":"2015","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_26","doi-asserted-by":"crossref","first-page":"1173","DOI":"10.1086\/587859","article-title":"Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657\u201356","volume":"679","author":"Randall","year":"2008","journal-title":"Astrophys. J."},{"key":"ref_27","doi-asserted-by":"crossref","first-page":"063506","DOI":"10.1103\/PhysRevD.94.063506","article-title":"Observational Constraints on Decoupled Hidden Sectors","volume":"94","author":"Heikinheimo","year":"2016","journal-title":"Phys. Rev. D"},{"key":"ref_28","doi-asserted-by":"crossref","first-page":"091304","DOI":"10.1103\/PhysRevLett.88.091304","article-title":"Thermally generated gauge singlet scalars as selfinteracting dark matter","volume":"88","author":"McDonald","year":"2002","journal-title":"Phys. Rev. Lett."},{"key":"ref_29","doi-asserted-by":"crossref","first-page":"80","DOI":"10.1007\/JHEP03(2010)080","article-title":"Freeze-In Production of FIMP Dark Matter","volume":"3","author":"Hall","year":"2010","journal-title":"J. High Energy Phys."},{"key":"ref_30","first-page":"1","article-title":"The Early Universe","volume":"69","author":"Kolb","year":"1990","journal-title":"Front. Phys."},{"key":"ref_31","doi-asserted-by":"crossref","first-page":"3637","DOI":"10.1103\/PhysRevD.50.3637","article-title":"Gauge singlet scalars as cold dark matter","volume":"50","author":"McDonald","year":"1994","journal-title":"Phys. Rev. D"},{"key":"ref_32","doi-asserted-by":"crossref","first-page":"709","DOI":"10.1016\/S0550-3213(01)00513-2","article-title":"The Minimal model of nonbaryonic dark matter: A Singlet scalar","volume":"619","author":"Burgess","year":"2001","journal-title":"Nucl. Phys. B"},{"key":"ref_33","doi-asserted-by":"crossref","first-page":"012","DOI":"10.1088\/1475-7516\/2013\/01\/012","article-title":"Electroweak baryogenesis and dark matter from a singlet Higgs","volume":"01","author":"Cline","year":"2013","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_34","doi-asserted-by":"crossref","first-page":"164","DOI":"10.1016\/0031-9163(65)90284-2","article-title":"Quarks, astrophysical and physico-chemical aspects","volume":"17","author":"Zeldovic","year":"1965","journal-title":"Phys. Lett."},{"key":"ref_35","doi-asserted-by":"crossref","first-page":"165","DOI":"10.1103\/PhysRevLett.39.165","article-title":"Cosmological Lower Bound on Heavy Neutrino Masses","volume":"39","author":"Lee","year":"1977","journal-title":"Phys. Rev. Lett."},{"key":"ref_36","doi-asserted-by":"crossref","first-page":"145","DOI":"10.1016\/0550-3213(91)90438-4","article-title":"Cosmic abundances of stable particles: Improved analysis","volume":"360","author":"Gondolo","year":"1991","journal-title":"Nucl. Phys. B"},{"key":"ref_37","doi-asserted-by":"crossref","first-page":"3191","DOI":"10.1103\/PhysRevD.43.3191","article-title":"Three exceptions in the calculation of relic abundances","volume":"43","author":"Griest","year":"1991","journal-title":"Phys. Rev. D"},{"key":"ref_38","doi-asserted-by":"crossref","first-page":"028","DOI":"10.1088\/1126-6708\/2009\/01\/028","article-title":"Hidden vector dark matter","volume":"01","author":"Hambye","year":"2009","journal-title":"J. High Energy Phys."},{"key":"ref_39","doi-asserted-by":"crossref","first-page":"061102","DOI":"10.1103\/PhysRevLett.119.061102","article-title":"Fourth Exception in the Calculation of Relic Abundances","volume":"119","author":"Pappadopulo","year":"2017","journal-title":"Phys. Rev. Lett."},{"key":"ref_40","doi-asserted-by":"crossref","first-page":"035","DOI":"10.1088\/1475-7516\/2014\/08\/035","article-title":"Standard Model with a real singlet scalar and inflation","volume":"08","author":"Enqvist","year":"2014","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_41","doi-asserted-by":"crossref","first-page":"065014","DOI":"10.1103\/PhysRevD.77.065014","article-title":"Dark-matter sterile neutrinos in models with a gauge singlet in the Higgs sector","volume":"77","author":"Petraki","year":"2008","journal-title":"Phys. Rev. D"},{"key":"ref_42","unstructured":"Dev, P.S.B., Mazumdar, A., and Qutub, S. (2014). Connection between dark matter abundance and primordial tensor perturbations. arXiv."},{"key":"ref_43","doi-asserted-by":"crossref","first-page":"001","DOI":"10.1088\/1475-7516\/2015\/11\/001","article-title":"Inflationary Imprints on Dark Matter","volume":"11","author":"Nurmi","year":"2015","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_44","doi-asserted-by":"crossref","first-page":"022","DOI":"10.1088\/1475-7516\/2016\/06\/022","article-title":"Isocurvature Constraints on Portal Couplings","volume":"06","author":"Kainulainen","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_45","doi-asserted-by":"crossref","first-page":"30","DOI":"10.1063\/1.2149672","article-title":"E-WIMPs","volume":"805","author":"Choi","year":"2005","journal-title":"AIP Conf. Proc."},{"key":"ref_46","doi-asserted-by":"crossref","first-page":"006","DOI":"10.1088\/1475-7516\/2012\/02\/006","article-title":"An intermediate framework between WIMP, FIMP, and EWIP dark matter","volume":"02","author":"Yaguna","year":"2012","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_47","doi-asserted-by":"crossref","first-page":"056","DOI":"10.1007\/JHEP02(2014)056","article-title":"Higher Dimensional Effective Operators for Direct Dark Matter Detection","volume":"2","author":"Krauss","year":"2014","journal-title":"J. High Energy Phys."},{"key":"ref_48","first-page":"1522","article-title":"On concentration of relict theta particles","volume":"31","author":"Dolgov","year":"1980","journal-title":"Yad. Fiz."},{"key":"ref_49","doi-asserted-by":"crossref","first-page":"43","DOI":"10.1086\/171833","article-title":"Self-interacting dark matter","volume":"398","author":"Carlson","year":"1992","journal-title":"Astrophys. J."},{"key":"ref_50","doi-asserted-by":"crossref","first-page":"034","DOI":"10.1088\/1475-7516\/2012\/05\/034","article-title":"The Four Basic Ways of Creating Dark Matter Through a Portal","volume":"05","author":"Chu","year":"2012","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_51","doi-asserted-by":"crossref","first-page":"115023","DOI":"10.1103\/PhysRevD.95.115023","article-title":"Simply split strongly interacting massive particles","volume":"95","author":"Bernal","year":"2017","journal-title":"Phys. Rev. D"},{"key":"ref_52","doi-asserted-by":"crossref","first-page":"055018","DOI":"10.1103\/PhysRevD.86.055018","article-title":"Regenerating WIMPs in the Light of Direct and Indirect Detection","volume":"86","author":"Williams","year":"2012","journal-title":"Phys. Rev. D"},{"key":"ref_53","doi-asserted-by":"crossref","first-page":"018","DOI":"10.1088\/1475-7516\/2016\/03\/018","article-title":"Production Regimes for Self-Interacting Dark Matter","volume":"03","author":"Bernal","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_54","doi-asserted-by":"crossref","first-page":"006","DOI":"10.1088\/1475-7516\/2016\/01\/006","article-title":"Z2 SIMP Dark Matter","volume":"01","author":"Bernal","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_55","doi-asserted-by":"crossref","first-page":"042","DOI":"10.1007\/JHEP03(2011)042","article-title":"Origins of Hidden Sector Dark Matter I: Cosmology","volume":"03","author":"Cheung","year":"2011","journal-title":"J. High Energy Phys."},{"key":"ref_56","doi-asserted-by":"crossref","first-page":"085","DOI":"10.1007\/JHEP03(2011)085","article-title":"Origins of Hidden Sector Dark Matter II: Collider Physics","volume":"03","author":"Cheung","year":"2011","journal-title":"J. High Energy Phys."},{"key":"ref_57","doi-asserted-by":"crossref","first-page":"182","DOI":"10.1016\/j.physletb.2015.11.025","article-title":"Cosmological Axion and neutrino mass constraints from Planck 2015 temperature and polarization data","volume":"752","author":"Giusarma","year":"2016","journal-title":"Phys. Lett. B"},{"key":"ref_58","first-page":"013","article-title":"Cosmological constraints in extended parameter space from the Planck 2018 Legacy release","volume":"01","author":"Melchiorri","year":"2020","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_59","doi-asserted-by":"crossref","first-page":"123008","DOI":"10.1103\/PhysRevD.84.123008","article-title":"The Case for Dark Radiation","volume":"84","author":"Archidiacono","year":"2011","journal-title":"Phys. Rev. D"},{"key":"ref_60","first-page":"051","article-title":"Relic neutrino decoupling with flavour oscillations revisited","volume":"07","author":"Pastor","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_61","doi-asserted-by":"crossref","first-page":"015004","DOI":"10.1103\/RevModPhys.88.015004","article-title":"Big Bang Nucleosynthesis: 2015","volume":"88","author":"Cyburt","year":"2016","journal-title":"Rev. Mod. Phys."},{"key":"ref_62","doi-asserted-by":"crossref","first-page":"023519","DOI":"10.1103\/PhysRevD.79.023519","article-title":"Dark Matter and Dark Radiation","volume":"79","author":"Ackerman","year":"2009","journal-title":"Phys. Rev. D"},{"key":"ref_63","doi-asserted-by":"crossref","first-page":"115021","DOI":"10.1103\/PhysRevD.96.115021","article-title":"Light Dark Matter: Models and Constraints","volume":"96","author":"Knapen","year":"2017","journal-title":"Phys. Rev. D"},{"key":"ref_64","doi-asserted-by":"crossref","first-page":"023004","DOI":"10.1103\/PhysRevD.100.023004","article-title":"Visualizing Invisible Dark Matter Annihilation with the CMB and Matter Power Spectrum","volume":"100","author":"Cui","year":"2019","journal-title":"Phys. Rev. D"},{"key":"ref_65","doi-asserted-by":"crossref","first-page":"629","DOI":"10.1038\/370629a0","article-title":"Evidence against dissipationless dark matter from observations of galaxy haloes","volume":"370","author":"Moore","year":"1994","journal-title":"Nature"},{"key":"ref_66","doi-asserted-by":"crossref","first-page":"L1","DOI":"10.1086\/187350","article-title":"Observational and theoretical constraints on singular dark matter halos","volume":"427","author":"Flores","year":"1994","journal-title":"Astrophys. J. Lett."},{"key":"ref_67","doi-asserted-by":"crossref","first-page":"493","DOI":"10.1086\/304888","article-title":"A Universal density profile from hierarchical clustering","volume":"490","author":"Navarro","year":"1997","journal-title":"Astrophys. J."},{"key":"ref_68","doi-asserted-by":"crossref","unstructured":"de Blok, W.J.G. (2010). The Core-Cusp Problem. Adv. Astron., 2010.","DOI":"10.1155\/2010\/789293"},{"key":"ref_69","doi-asserted-by":"crossref","first-page":"24","DOI":"10.1088\/0004-6256\/142\/1\/24","article-title":"The central slope of dark matter cores in dwarf galaxies: Simulations vs. THINGS","volume":"142","author":"Oh","year":"2011","journal-title":"Astron. J."},{"key":"ref_70","doi-asserted-by":"crossref","first-page":"20","DOI":"10.1088\/0004-637X\/742\/1\/20","article-title":"A Method for Measuring (Slopes of) the Mass Profiles of Dwarf Spheroidal Galaxies","volume":"742","author":"Walker","year":"2011","journal-title":"Astrophys. J."},{"key":"ref_71","doi-asserted-by":"crossref","first-page":"L40","DOI":"10.1111\/j.1745-3933.2011.01074.x","article-title":"Too big to fail? The puzzling darkness of massive Milky Way subhaloes","volume":"415","author":"Bullock","year":"2011","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_72","doi-asserted-by":"crossref","first-page":"222","DOI":"10.1093\/mnras\/stu1477","article-title":"Too Big to Fail in the Local Group","volume":"444","author":"Bullock","year":"2014","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_73","doi-asserted-by":"crossref","first-page":"142","DOI":"10.1086\/306832","article-title":"Starburst\u2013driven mass loss from dwarf galaxies: Efficiency and metal ejection","volume":"513","author":"Ferrara","year":"1999","journal-title":"Astrophys. J."},{"key":"ref_74","doi-asserted-by":"crossref","first-page":"203","DOI":"10.1038\/nature08640","article-title":"At the heart of the matter: The origin of bulgeless dwarf galaxies and Dark Matter cores","volume":"463","author":"Governato","year":"2010","journal-title":"Nature"},{"key":"ref_75","doi-asserted-by":"crossref","first-page":"556","DOI":"10.1088\/0004-637X\/725\/1\/556","article-title":"The massive black hole-velocity dispersion relation and the halo baryon fraction: A case for positive AGN feedback","volume":"725","author":"Silk","year":"2010","journal-title":"Astrophys. J."},{"key":"ref_76","doi-asserted-by":"crossref","first-page":"1696","DOI":"10.1093\/mnras\/sts148","article-title":"Not too big, not too small: The dark halos of the dwarf spheroidals in the Milky Way","volume":"428","author":"Helmi","year":"2013","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_77","doi-asserted-by":"crossref","first-page":"1931","DOI":"10.1093\/mnras\/stw145","article-title":"The APOSTLE simulations: Solutions to the Local Group\u2019s cosmic puzzles","volume":"457","author":"Sawala","year":"2016","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_78","unstructured":"Fattahi, A., Navarro, J.F., Sawala, T., Frenk, C.S., Sales, L.V., Oman, K., Schaller, M., and Wang, J. (2016). The cold dark matter content of Galactic dwarf spheroidals: No cores, no failures, no problem. arXiv."},{"key":"ref_79","doi-asserted-by":"crossref","first-page":"819","DOI":"10.1086\/383178","article-title":"Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56","volume":"606","author":"Markevitch","year":"2004","journal-title":"Astrophys. J."},{"key":"ref_80","doi-asserted-by":"crossref","first-page":"1462","DOI":"10.1126\/science.1261381","article-title":"The non-gravitational interactions of dark matter in colliding galaxy clusters","volume":"347","author":"Harvey","year":"2015","journal-title":"Science"},{"key":"ref_81","doi-asserted-by":"crossref","first-page":"569","DOI":"10.1093\/mnras\/stw2670","article-title":"What does the Bullet Cluster tell us about self-interacting dark matter?","volume":"465","author":"Robertson","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_82","doi-asserted-by":"crossref","first-page":"1414","DOI":"10.1093\/mnras\/stx896","article-title":"In the Wake of Dark Giants: New Signatures of Dark Matter Self Interactions in Equal Mass Mergers of Galaxy Clusters","volume":"469","author":"Kim","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_83","doi-asserted-by":"crossref","first-page":"4719","DOI":"10.1093\/mnras\/stx463","article-title":"Cosmic particle colliders: Simulations of self-interacting dark matter with anisotropic scattering","volume":"467","author":"Robertson","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_84","doi-asserted-by":"crossref","first-page":"104","DOI":"10.3847\/1538-4357\/aaee77","article-title":"The Mismeasure of Mergers: Revised Limits on Self-interacting Dark Matter in Merging Galaxy Clusters","volume":"869","author":"Wittman","year":"2018","journal-title":"Astrophys. J."},{"key":"ref_85","doi-asserted-by":"crossref","first-page":"3393","DOI":"10.1093\/mnras\/stv467","article-title":"The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827","volume":"449","author":"Massey","year":"2015","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_86","doi-asserted-by":"crossref","first-page":"L54","DOI":"10.1093\/mnrasl\/slv088","article-title":"On the interpretation of dark matter self-interactions in Abell 3827","volume":"452","author":"Kahlhoefer","year":"2015","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_87","doi-asserted-by":"crossref","first-page":"5004","DOI":"10.1093\/mnras\/stx855","article-title":"A test for skewed distributions of dark matter and a possible detection in galaxy cluster Abell 3827","volume":"468","author":"Taylor","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_88","doi-asserted-by":"crossref","first-page":"115007","DOI":"10.1103\/PhysRevD.87.115007","article-title":"Beyond Collisionless Dark Matter: Particle Physics Dynamics for Dark Matter Halo Structure","volume":"87","author":"Tulin","year":"2013","journal-title":"Phys. Rev. D"},{"key":"ref_89","doi-asserted-by":"crossref","first-page":"035009","DOI":"10.1103\/PhysRevD.89.035009","article-title":"Direct Detection Portals for Self-interacting Dark Matter","volume":"89","author":"Kaplinghat","year":"2014","journal-title":"Phys. Rev. D"},{"key":"ref_90","doi-asserted-by":"crossref","first-page":"76","DOI":"10.1016\/j.physletb.2018.06.024","article-title":"Signatures of Self-Interacting Dark Matter in the Matter Power Spectrum and the CMB","volume":"783","author":"Huo","year":"2018","journal-title":"Phys. Lett. B"},{"key":"ref_91","first-page":"013","article-title":"The Cosmological Evolution of Self-interacting Dark Matter","volume":"05","author":"Essig","year":"2021","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_92","doi-asserted-by":"crossref","first-page":"041","DOI":"10.1088\/1475-7516\/2013\/08\/041","article-title":"A Lower Bound on the Mass of Cold Thermal Dark Matter from Planck","volume":"08","author":"Boehm","year":"2013","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_93","doi-asserted-by":"crossref","first-page":"083508","DOI":"10.1103\/PhysRevD.89.083508","article-title":"BBN And The CMB Constrain Light, Electromagnetically Coupled WIMPs","volume":"89","author":"Nollett","year":"2014","journal-title":"Phys. Rev. D"},{"key":"ref_94","doi-asserted-by":"crossref","first-page":"043526","DOI":"10.1103\/PhysRevD.80.043526","article-title":"CMB Constraints on WIMP Annihilation: Energy Absorption During the Recombination Epoch","volume":"80","author":"Slatyer","year":"2009","journal-title":"Phys. Rev. D"},{"key":"ref_95","unstructured":"Goodenough, L., and Hooper, D. (2009). Possible Evidence For Dark Matter Annihilation In The Inner Milky Way From The Fermi Gamma Ray Space Telescope. arXiv."},{"key":"ref_96","doi-asserted-by":"crossref","first-page":"083511","DOI":"10.1103\/PhysRevD.86.083511","article-title":"Detection of a Gamma-Ray Source in the Galactic Center Consistent with Extended Emission from Dark Matter Annihilation and Concentrated Astrophysical Emission","volume":"86","author":"Abazajian","year":"2012","journal-title":"Phys. Rev. D"},{"key":"ref_97","doi-asserted-by":"crossref","first-page":"1","DOI":"10.1016\/j.dark.2015.12.005","article-title":"The characterization of the gamma-ray signal from the central Milky Way: A case for annihilating dark matter","volume":"12","author":"Daylan","year":"2016","journal-title":"Phys. Dark Univ."},{"key":"ref_98","doi-asserted-by":"crossref","first-page":"123010","DOI":"10.1103\/PhysRevD.91.123010","article-title":"GeV excess in the Milky Way: The role of diffuse galactic gamma-ray emission templates","volume":"91","author":"Zhou","year":"2015","journal-title":"Phys. Rev. D"},{"key":"ref_99","doi-asserted-by":"crossref","first-page":"38","DOI":"10.1088\/1475-7516\/2015\/03\/038","article-title":"Background Model Systematics for the Fermi GeV Excess","volume":"3","author":"Calore","year":"2015","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_100","doi-asserted-by":"crossref","first-page":"44","DOI":"10.3847\/0004-637X\/819\/1\/44","article-title":"Fermi-LAT Observations of High-Energy \u03b3-Ray Emission Toward the Galactic Center","volume":"819","author":"Ajello","year":"2016","journal-title":"Astrophys. J."},{"key":"ref_101","doi-asserted-by":"crossref","first-page":"103013","DOI":"10.1103\/PhysRevD.94.103013","article-title":"High-energy tail of the Galactic Center gamma-ray excess","volume":"94","author":"Linden","year":"2016","journal-title":"Phys. Rev. D"},{"key":"ref_102","first-page":"052","article-title":"Galactic Center gamma-ray \u201cexcess\u201d from an active past of the Galactic Centre?","volume":"10","author":"Serpico","year":"2014","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_103","doi-asserted-by":"crossref","first-page":"1","DOI":"10.1088\/0004-637X\/796\/1\/14","article-title":"Diffuse gamma-ray emission from galactic pulsars","volume":"796","author":"Calore","year":"2014","journal-title":"Astrophys. J."},{"key":"ref_104","doi-asserted-by":"crossref","first-page":"043","DOI":"10.1088\/1475-7516\/2015\/06\/043","article-title":"Challenges in Explaining the Galactic Center Gamma-Ray Excess with Millisecond Pulsars","volume":"06","author":"Cholis","year":"2015","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_105","first-page":"023","article-title":"Millisecond pulsars and the Galactic Center gamma-ray excess: The importance of luminosity function and secondary emission","volume":"02","author":"Serpico","year":"2015","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_106","doi-asserted-by":"crossref","first-page":"005","DOI":"10.1088\/1475-7516\/2015\/12\/005","article-title":"The Galactic Center GeV Excess from a Series of Leptonic Cosmic-Ray Outbursts","volume":"12","author":"Cholis","year":"2015","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_107","doi-asserted-by":"crossref","first-page":"387","DOI":"10.1038\/s41550-018-0414-3","article-title":"Galactic bulge preferred over dark matter for the Galactic centre gamma-ray excess","volume":"2","author":"Macias","year":"2018","journal-title":"Nat. Astron."},{"key":"ref_108","doi-asserted-by":"crossref","first-page":"063003","DOI":"10.1103\/PhysRevD.91.063003","article-title":"A Tale of Tails: Dark Matter Interpretations of the Fermi GeV Excess in Light of Background Model Systematics","volume":"91","author":"Calore","year":"2015","journal-title":"Phys. Rev. D"},{"key":"ref_109","doi-asserted-by":"crossref","first-page":"037","DOI":"10.1088\/1475-7516\/2016\/04\/037","article-title":"Global analysis of the pMSSM in light of the Fermi GeV excess: Prospects for the LHC Run-II and astroparticle experiments","volume":"04","author":"Bertone","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_110","doi-asserted-by":"crossref","first-page":"110","DOI":"10.3847\/1538-4357\/834\/2\/110","article-title":"Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-LAT","volume":"834","author":"Albert","year":"2017","journal-title":"Astrophys. J."},{"key":"ref_111","doi-asserted-by":"crossref","first-page":"091103","DOI":"10.1103\/PhysRevLett.117.091103","article-title":"Antiproton Flux, Antiproton-to-Proton Flux Ratio, and Properties of Elementary Particle Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station","volume":"117","author":"Aguilar","year":"2016","journal-title":"Phys. Rev. Lett."},{"key":"ref_112","doi-asserted-by":"crossref","unstructured":"Cui, M.Y., Yuan, Q., Tsai, Y.L.S., and Fan, Y.Z. (2017). Novel Dark Matter Constraints from Antiprotons in Light of AMS-02. Phys. Rev. Lett., 118.","DOI":"10.1103\/PhysRevLett.118.191101"},{"key":"ref_113","doi-asserted-by":"crossref","unstructured":"Cui, M.Y., Yuan, Q., Tsai, Y.L.S., and Fan, Y.Z. (2017). Possible dark matter annihilation signal in the AMS-02 antiproton data. Phys. Rev. Lett., 118.","DOI":"10.1103\/PhysRevLett.118.191101"},{"key":"ref_114","doi-asserted-by":"crossref","first-page":"063021","DOI":"10.1103\/PhysRevD.95.063021","article-title":"Antiprotons from dark matter annihilation through light mediators and a possible excess in AMS-02 p\u00af\/p data","volume":"95","author":"Huang","year":"2017","journal-title":"Phys. Rev. D"},{"key":"ref_115","doi-asserted-by":"crossref","first-page":"112","DOI":"10.1007\/JHEP04(2017)112","article-title":"Simplified dark matter models in the light of AMS-02 antiproton data","volume":"04","author":"Li","year":"2017","journal-title":"J. High Energy Phys."},{"key":"ref_116","doi-asserted-by":"crossref","first-page":"116","DOI":"10.3847\/1538-4357\/aabf87","article-title":"Dark Matter Search in Space: Combined Analysis of Cosmic Ray Antiproton-to-Proton Flux Ratio and Positron Flux Measured by AMS-02","volume":"858","author":"Feng","year":"2018","journal-title":"Astrophys. J."},{"key":"ref_117","doi-asserted-by":"crossref","first-page":"80","DOI":"10.3847\/1538-4357\/abb01a","article-title":"Astrophysical background and dark matter implication based on latest AMS-02 data","volume":"901","author":"Jin","year":"2020","journal-title":"Astrophys. J."},{"key":"ref_118","doi-asserted-by":"crossref","first-page":"055009","DOI":"10.1103\/PhysRevD.96.055009","article-title":"Interpretation of the gamma-ray excess and AMS-02 antiprotons: Velocity dependent dark matter annihilations","volume":"96","author":"Jia","year":"2017","journal-title":"Phys. Rev. D"},{"key":"ref_119","doi-asserted-by":"crossref","first-page":"053","DOI":"10.1088\/1475-7516\/2017\/10\/053","article-title":"Probing dark matter annihilation in the Galaxy with antiprotons and gamma rays","volume":"10","author":"Cuoco","year":"2017","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_120","doi-asserted-by":"crossref","first-page":"123005","DOI":"10.1103\/PhysRevD.103.123005","article-title":"Multimessenger constraints on the dark matter interpretation of the Fermi-LAT Galactic center excess","volume":"103","author":"Winkler","year":"2021","journal-title":"Phys. Rev. D"},{"key":"ref_121","doi-asserted-by":"crossref","first-page":"23","DOI":"10.1088\/1475-7516\/2015\/09\/023","article-title":"AMS-02 antiprotons, at last! Secondary astrophysical component and immediate implications for Dark Matter","volume":"9","author":"Giesen","year":"2015","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_122","doi-asserted-by":"crossref","first-page":"607","DOI":"10.1038\/nature07942","article-title":"An anomalous positron abundance in cosmic rays with energies 1.5\u2013100 GeV","volume":"458","author":"Adriani","year":"2009","journal-title":"Nature"},{"key":"ref_123","doi-asserted-by":"crossref","first-page":"141102","DOI":"10.1103\/PhysRevLett.110.141102","article-title":"First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5\u2013350 GeV","volume":"110","author":"Aguilar","year":"2013","journal-title":"Phys. Rev. Lett."},{"key":"ref_124","doi-asserted-by":"crossref","first-page":"25","DOI":"10.1088\/1475-7516\/2009\/01\/025","article-title":"Pulsars as the Sources of High Energy Cosmic Ray Positrons","volume":"1","author":"Hooper","year":"2009","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_125","first-page":"006","article-title":"Interpretation of AMS-02 electrons and positrons data","volume":"04","author":"Donato","year":"2014","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_126","doi-asserted-by":"crossref","first-page":"055004","DOI":"10.1103\/PhysRevD.80.055004","article-title":"The PAMELA excess from neutralino annihilation in the NMSSM","volume":"80","author":"Bai","year":"2009","journal-title":"Phys. Rev. D"},{"key":"ref_127","doi-asserted-by":"crossref","first-page":"495","DOI":"10.1016\/j.physletb.2015.06.035","article-title":"Dark matter for excess of AMS-02 positrons and antiprotons","volume":"747","author":"Chen","year":"2015","journal-title":"Phys. Lett. B"},{"key":"ref_128","doi-asserted-by":"crossref","first-page":"136","DOI":"10.1016\/0370-2693(85)90624-0","article-title":"Scalar phantoms","volume":"161","author":"Silveira","year":"1985","journal-title":"Phys. Lett. B"},{"key":"ref_129","unstructured":"Patt, B., and Wilczek, F. (2006). Higgs-field portal into hidden sectors. arXiv."},{"key":"ref_130","doi-asserted-by":"crossref","first-page":"075028","DOI":"10.1103\/PhysRevD.99.075028","article-title":"Direct and indirect probes of Goldstone dark matter","volume":"99","author":"Alanne","year":"2019","journal-title":"Phys. Rev. D"},{"key":"ref_131","doi-asserted-by":"crossref","first-page":"115012","DOI":"10.1103\/PhysRevD.75.115012","article-title":"The Minimal model of fermionic dark matter","volume":"75","author":"Kim","year":"2007","journal-title":"Phys. Rev. D"},{"key":"ref_132","doi-asserted-by":"crossref","first-page":"100","DOI":"10.1063\/1.2896759","article-title":"Singlet fermionic dark matter","volume":"5","author":"Kim","year":"2008","journal-title":"J. High Energy Phys."},{"key":"ref_133","doi-asserted-by":"crossref","first-page":"39","DOI":"10.1016\/j.physletb.2009.11.050","article-title":"Confined hidden vector dark matter","volume":"683","author":"Hambye","year":"2010","journal-title":"Phys. Lett. B"},{"key":"ref_134","doi-asserted-by":"crossref","first-page":"196","DOI":"10.1016\/0370-2693(86)91377-8","article-title":"Two U(1)\u2019s and Epsilon Charge Shifts","volume":"166","author":"Holdom","year":"1986","journal-title":"Phys. Lett. B"},{"key":"ref_135","first-page":"172","article-title":"A force beyond the Standard Model - Status of the quest for hidden photons","volume":"56","author":"Jaeckel","year":"2012","journal-title":"Frascati Phys. Ser."},{"key":"ref_136","unstructured":"Fabbrichesi, M., Gabrielli, E., and Lanfranchi, G. (2021). The Dark Photon, Springer."},{"key":"ref_137","doi-asserted-by":"crossref","first-page":"063509","DOI":"10.1103\/PhysRevD.83.063509","article-title":"Turning off the Lights: How Dark is Dark Matter?","volume":"83","author":"McDermott","year":"2011","journal-title":"Phys. Rev. D"},{"key":"ref_138","doi-asserted-by":"crossref","first-page":"023519","DOI":"10.1103\/PhysRevD.89.023519","article-title":"Constraining Dark Matter-Baryon Scattering with Linear Cosmology","volume":"89","author":"Dvorkin","year":"2014","journal-title":"Phys. Rev. D"},{"key":"ref_139","doi-asserted-by":"crossref","unstructured":"Caputo, A., Millar, A.J., O\u2019Hare, C.A.J., and Vitagliano, E. (2021). Dark photon limits: A cookbook. arXiv.","DOI":"10.1103\/PhysRevD.104.095029"},{"key":"ref_140","doi-asserted-by":"crossref","first-page":"1440","DOI":"10.1103\/PhysRevLett.38.1440","article-title":"CP Conservation in the Presence of Instantons","volume":"38","author":"Peccei","year":"1977","journal-title":"Phys. Rev. Lett."},{"key":"ref_141","doi-asserted-by":"crossref","first-page":"1791","DOI":"10.1103\/PhysRevD.16.1791","article-title":"Constraints Imposed by CP Conservation in the Presence of Instantons","volume":"16","author":"Peccei","year":"1977","journal-title":"Phys. Rev. D"},{"key":"ref_142","doi-asserted-by":"crossref","first-page":"199","DOI":"10.1016\/0370-2693(81)90590-6","article-title":"A Simple Solution to the Strong CP Problem with a Harmless Axion","volume":"104","author":"Dine","year":"1981","journal-title":"Phys. Lett. B"},{"key":"ref_143","first-page":"260","article-title":"On Possible Suppression of the Axion Hadron Interactions","volume":"31","author":"Zhitnitsky","year":"1980","journal-title":"Sov. J. Nucl. Phys."},{"key":"ref_144","doi-asserted-by":"crossref","first-page":"103","DOI":"10.1103\/PhysRevLett.43.103","article-title":"Weak Interaction Singlet and Strong CP Invariance","volume":"43","author":"Kim","year":"1979","journal-title":"Phys. Rev. Lett."},{"key":"ref_145","doi-asserted-by":"crossref","first-page":"493","DOI":"10.1016\/0550-3213(80)90209-6","article-title":"Can Confinement Ensure Natural CP Invariance of Strong Interactions?","volume":"166","author":"Shifman","year":"1980","journal-title":"Nucl. Phys. B"},{"key":"ref_146","doi-asserted-by":"crossref","first-page":"127","DOI":"10.1016\/0370-2693(83)90637-8","article-title":"Cosmology of the Invisible Axion","volume":"120","author":"Preskill","year":"1983","journal-title":"Phys. Lett. B"},{"key":"ref_147","doi-asserted-by":"crossref","first-page":"133","DOI":"10.1016\/0370-2693(83)90638-X","article-title":"A Cosmological Bound on the Invisible Axion","volume":"120","author":"Abbott","year":"1983","journal-title":"Phys. Lett. B"},{"key":"ref_148","doi-asserted-by":"crossref","unstructured":"Choi, K., Im, S.H., and Shin, C.S. (2021). Recent progress in physics of axions or axion-like particles. Annu. Rev. Nucl. Part. Sci.","DOI":"10.1146\/annurev-nucl-120720-031147"},{"key":"ref_149","doi-asserted-by":"crossref","first-page":"113","DOI":"10.1007\/JHEP06(2010)113","article-title":"The Cosmology of Composite Inelastic Dark Matter","volume":"06","author":"Alves","year":"2010","journal-title":"J. High Energy Phys."},{"key":"ref_150","doi-asserted-by":"crossref","first-page":"095001","DOI":"10.1103\/PhysRevD.81.095001","article-title":"Quirky Composite Dark Matter","volume":"81","author":"Kribs","year":"2010","journal-title":"Phys. Rev. D"},{"key":"ref_151","doi-asserted-by":"crossref","first-page":"055034","DOI":"10.1103\/PhysRevD.92.055034","article-title":"Twin Higgs WIMP Dark Matter","volume":"92","author":"Lasenby","year":"2015","journal-title":"Phys. Rev. D"},{"key":"ref_152","doi-asserted-by":"crossref","first-page":"111701","DOI":"10.1103\/PhysRevD.82.111701","article-title":"Weakly Interacting Stable Pions","volume":"82","author":"Bai","year":"2010","journal-title":"Phys. Rev. D"},{"key":"ref_153","doi-asserted-by":"crossref","first-page":"115","DOI":"10.1007\/JHEP02(2014)115","article-title":"Pionic Dark Matter","volume":"2","author":"Bhattacharya","year":"2014","journal-title":"J. High Energy Phys."},{"key":"ref_154","doi-asserted-by":"crossref","first-page":"262","DOI":"10.1016\/j.physletb.2010.12.047","article-title":"Electroweak symmetry breaking and cold dark matter from strongly interacting hidden sector","volume":"696","author":"Hur","year":"2011","journal-title":"Phys. Lett. B"},{"key":"ref_155","doi-asserted-by":"crossref","first-page":"1450077","DOI":"10.1142\/S0217732314500771","article-title":"Physical Naturalness and Dynamical Breaking of Classical Scale Invariance","volume":"29","author":"Heikinheimo","year":"2014","journal-title":"Mod. Phys. Lett. A"},{"key":"ref_156","doi-asserted-by":"crossref","first-page":"060","DOI":"10.1007\/JHEP04(2013)060","article-title":"Emergence of the Electroweak Scale through the Higgs Portal","volume":"4","author":"Englert","year":"2013","journal-title":"J. High Energy Phys."},{"key":"ref_157","doi-asserted-by":"crossref","first-page":"015","DOI":"10.1007\/JHEP07(2012)015","article-title":"Composite Scalar Dark Matter","volume":"07","author":"Frigerio","year":"2012","journal-title":"J. High Energy Phys."},{"key":"ref_158","doi-asserted-by":"crossref","first-page":"95","DOI":"10.1016\/0370-2693(71)90582-X","article-title":"Consequences of anomalous Ward identities","volume":"37","author":"Wess","year":"1971","journal-title":"Phys. Lett. B"},{"key":"ref_159","doi-asserted-by":"crossref","first-page":"422","DOI":"10.1016\/0550-3213(83)90063-9","article-title":"Global Aspects of Current Algebra","volume":"223","author":"Witten","year":"1983","journal-title":"Nucl. Phys. B"},{"key":"ref_160","doi-asserted-by":"crossref","first-page":"055002","DOI":"10.1103\/PhysRevD.103.055002","article-title":"Singlet dark matter in the SU(6)\/SO(6) composite Higgs model","volume":"103","author":"Cai","year":"2021","journal-title":"Phys. Rev. D"},{"key":"ref_161","doi-asserted-by":"crossref","first-page":"095021","DOI":"10.1103\/PhysRevD.91.095021","article-title":"Elementary Goldstone Higgs boson and dark matter","volume":"91","author":"Alanne","year":"2015","journal-title":"Phys. Rev. D"},{"key":"ref_162","doi-asserted-by":"crossref","first-page":"075015","DOI":"10.1103\/PhysRevD.94.075015","article-title":"Vacuum alignment with and without elementary scalars","volume":"94","author":"Alanne","year":"2016","journal-title":"Phys. Rev. D"},{"key":"ref_163","doi-asserted-by":"crossref","first-page":"043510","DOI":"10.1103\/PhysRevD.87.043510","article-title":"Thermal dark matter from a confining sector","volume":"87","author":"Buckley","year":"2013","journal-title":"Phys. Rev. D"},{"key":"ref_164","doi-asserted-by":"crossref","first-page":"323","DOI":"10.1016\/j.physletb.2010.08.006","article-title":"Composite Inelastic Dark Matter","volume":"692","author":"Alves","year":"2010","journal-title":"Phys. Lett. B"},{"key":"ref_165","doi-asserted-by":"crossref","first-page":"043502","DOI":"10.1103\/PhysRevD.64.043502","article-title":"Inelastic dark matter","volume":"64","author":"Weiner","year":"2001","journal-title":"Phys. Rev. D"},{"key":"ref_166","doi-asserted-by":"crossref","first-page":"063509","DOI":"10.1103\/PhysRevD.72.063509","article-title":"The Status of inelastic dark matter","volume":"72","author":"Weiner","year":"2005","journal-title":"Phys. Rev. D"},{"key":"ref_167","doi-asserted-by":"crossref","first-page":"043513","DOI":"10.1103\/PhysRevD.79.043513","article-title":"Inelastic Dark Matter in Light of DAMA\/LIBRA","volume":"79","author":"Chang","year":"2009","journal-title":"Phys. Rev. D"},{"key":"ref_168","doi-asserted-by":"crossref","first-page":"065","DOI":"10.1088\/1126-6708\/2009\/11\/065","article-title":"Macroscopic Strings and \u2019Quirks\u2019 at Colliders","volume":"11","author":"Kang","year":"2009","journal-title":"J. High Energy Phys."},{"key":"ref_169","doi-asserted-by":"crossref","first-page":"197","DOI":"10.1016\/0550-3213(80)90051-6","article-title":"The Alignment of the Vacuum in Theories of Technicolor","volume":"175","author":"Peskin","year":"1980","journal-title":"Nucl. Phys. B"},{"key":"ref_170","doi-asserted-by":"crossref","first-page":"035029","DOI":"10.1103\/PhysRevD.84.035029","article-title":"Quirks at the Tevatron and Beyond","volume":"84","author":"Harnik","year":"2011","journal-title":"Phys. Rev. D"},{"key":"ref_171","doi-asserted-by":"crossref","first-page":"445","DOI":"10.1016\/0550-3213(90)90151-3","article-title":"TECHNICOLOR COSMOLOGY","volume":"329","author":"Chivukula","year":"1990","journal-title":"Nucl. Phys. B"},{"key":"ref_172","doi-asserted-by":"crossref","first-page":"095008","DOI":"10.1103\/PhysRevD.74.095008","article-title":"Dark Matter from new Technicolor Theories","volume":"74","author":"Gudnason","year":"2006","journal-title":"Phys. Rev. D"},{"key":"ref_173","doi-asserted-by":"crossref","first-page":"387","DOI":"10.1016\/0370-2693(90)91661-T","article-title":"Electroweak Fermion Number Violation and the Production of Stable Particles in the Early Universe","volume":"241","author":"Barr","year":"1990","journal-title":"Phys. Lett. B"},{"key":"ref_174","doi-asserted-by":"crossref","first-page":"741","DOI":"10.1103\/PhysRevLett.68.741","article-title":"A Single explanation for both the baryon and dark matter densities","volume":"68","author":"Kaplan","year":"1992","journal-title":"Phys. Rev. Lett."},{"key":"ref_175","doi-asserted-by":"crossref","first-page":"451","DOI":"10.1016\/S0927-6505(01)00121-9","article-title":"Selfinteracting dark matter from the hidden heterotic string sector","volume":"16","author":"Faraggi","year":"2002","journal-title":"Astropart. Phys."},{"key":"ref_176","doi-asserted-by":"crossref","first-page":"179","DOI":"10.1016\/j.physletb.2012.07.017","article-title":"Higgs portal, fermionic dark matter, and a Standard Model like Higgs at 125 GeV","volume":"716","author":"Schwetz","year":"2012","journal-title":"Phys. Lett. B"},{"key":"ref_177","doi-asserted-by":"crossref","first-page":"2455","DOI":"10.1140\/epjc\/s10052-013-2455-1","article-title":"Direct Detection of Higgs-Portal Dark Matter at the LHC","volume":"73","author":"Djouadi","year":"2013","journal-title":"Eur. Phys. J. C"},{"key":"ref_178","unstructured":"Brooijmans, G., Gripaios, B., Moortgat, F., Santiago, J., Skands, P., Albornoz V\u00e1squez, D., Allanach, B.C., Alloul, A., Arbey, A., and Azatov, A. (2012). Les Houches 2011: Physics at TeV Colliders New Physics Working Group Report. arXiv."},{"key":"ref_179","doi-asserted-by":"crossref","first-page":"005","DOI":"10.1088\/1475-7516\/2013\/08\/005","article-title":"Minimal Decaying Dark Matter and the LHC","volume":"08","author":"Arcadi","year":"2013","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_180","doi-asserted-by":"crossref","first-page":"647","DOI":"10.1016\/j.physletb.2016.07.042","article-title":"Search for heavy long-lived charged R-hadrons with the ATLAS detector in 3.2 fb\u22121 of proton\u2013proton collision data at s = 13 TeV","volume":"760","author":"Aaboud","year":"2016","journal-title":"Phys. Lett. B"},{"key":"ref_181","doi-asserted-by":"crossref","first-page":"112004","DOI":"10.1103\/PhysRevD.94.112004","article-title":"Search for long-lived charged particles in proton-proton collisions at s = 13 TeV","volume":"94","author":"Khachatryan","year":"2016","journal-title":"Phys. Rev. D"},{"key":"ref_182","doi-asserted-by":"crossref","first-page":"015","DOI":"10.1088\/1475-7516\/2014\/07\/015","article-title":"FIMP realization of the scotogenic model","volume":"07","author":"Molinaro","year":"2014","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_183","doi-asserted-by":"crossref","first-page":"095006","DOI":"10.1088\/0954-3899\/43\/9\/095006","article-title":"Freeze-in production of Fermionic Dark Matter with Pseudo-scalar and Phenomenological Aspects","volume":"43","author":"Firouzabadi","year":"2016","journal-title":"J. Phys. G"},{"key":"ref_184","doi-asserted-by":"crossref","first-page":"100","DOI":"10.1007\/JHEP01(2017)100","article-title":"Probing the scotogenic FIMP at the LHC","volume":"1","author":"Hessler","year":"2017","journal-title":"J. High Energy Phys."},{"key":"ref_185","doi-asserted-by":"crossref","first-page":"1830007","DOI":"10.1142\/S0217732318300070","article-title":"Constraining Extended Scalar Sectors at the LHC and beyond","volume":"33","author":"Ilnicka","year":"2018","journal-title":"Mod. Phys. Lett. A"},{"key":"ref_186","doi-asserted-by":"crossref","first-page":"206","DOI":"10.1007\/JHEP11(2015)206","article-title":"Constraints on new phenomena via Higgs boson couplings and invisible decays with the ATLAS detector","volume":"11","author":"Aad","year":"2015","journal-title":"J. High Energy Phys."},{"key":"ref_187","doi-asserted-by":"crossref","first-page":"135","DOI":"10.1007\/JHEP02(2017)135","article-title":"Searches for invisible decays of the Higgs boson in pp collisions at s = 7, 8, and 13 TeV","volume":"2","author":"Khachatryan","year":"2017","journal-title":"J. High Energy Phys."},{"key":"ref_188","doi-asserted-by":"crossref","first-page":"39","DOI":"10.1140\/epjc\/s10052-010-1303-9","article-title":"New results from DAMA\/LIBRA","volume":"67","author":"Bernabei","year":"2010","journal-title":"Eur. Phys. J. C"},{"key":"ref_189","doi-asserted-by":"crossref","first-page":"2648","DOI":"10.1140\/epjc\/s10052-013-2648-7","article-title":"Final model independent result of DAMA\/LIBRA-phase1","volume":"73","author":"Bernabei","year":"2013","journal-title":"Eur. Phys. J. C"},{"key":"ref_190","doi-asserted-by":"crossref","first-page":"131301","DOI":"10.1103\/PhysRevLett.106.131301","article-title":"Results from a Search for Light-Mass Dark Matter with a P-type Point Contact Germanium Detector","volume":"106","author":"Aalseth","year":"2011","journal-title":"Phys. Rev. Lett."},{"key":"ref_191","doi-asserted-by":"crossref","first-page":"141301","DOI":"10.1103\/PhysRevLett.107.141301","article-title":"Search for an Annual Modulation in a P-type Point Contact Germanium Dark Matter Detector","volume":"107","author":"Aalseth","year":"2011","journal-title":"Phys. Rev. Lett."},{"key":"ref_192","doi-asserted-by":"crossref","first-page":"012002","DOI":"10.1103\/PhysRevD.88.012002","article-title":"CoGeNT: A Search for Low-Mass Dark Matter using p-type Point Contact Germanium Detectors","volume":"88","author":"Aalseth","year":"2013","journal-title":"Phys. Rev. D"},{"key":"ref_193","unstructured":"Aalseth, C.E., Barbeau, P.S., Colaresi, J., Collar, J.I., Leon, J.D., Fast, J.E., Fields, N.E., Hossbach, T.W., Knecht, A., and Kos, M.S. (2014). Search for An Annual Modulation in Three Years of CoGeNT Dark Matter Detector Data. arXiv."},{"key":"ref_194","unstructured":"Aalseth, C.E., Barbeau, P.S., Colaresi, J., Leon, J.D., Fast, J.E., Hossbach, T.W., Knecht, A., Kos, M.S., Marino, M.G., and Miley, H.S. (2014). Maximum Likelihood Signal Extraction Method Applied to 3.4 years of CoGeNT Data. arXiv."},{"key":"ref_195","doi-asserted-by":"crossref","first-page":"251301","DOI":"10.1103\/PhysRevLett.111.251301","article-title":"Silicon Detector Dark Matter Results from the Final Exposure of CDMS II","volume":"111","author":"Agnese","year":"2013","journal-title":"Phys. Rev. Lett."},{"key":"ref_196","doi-asserted-by":"crossref","first-page":"021303","DOI":"10.1103\/PhysRevLett.118.021303","article-title":"Results from a search for dark matter in the complete LUX exposure","volume":"118","author":"Akerib","year":"2017","journal-title":"Phys. Rev. Lett."},{"key":"ref_197","doi-asserted-by":"crossref","first-page":"111302","DOI":"10.1103\/PhysRevLett.121.111302","article-title":"Dark Matter Search Results from a One Ton-Year Exposure of XENON1T","volume":"121","author":"Aprile","year":"2018","journal-title":"Phys. Rev. Lett."},{"key":"ref_198","first-page":"040","article-title":"Precision calculations of dark matter relic abundance","volume":"09","author":"Kainulainen","year":"2020","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_199","doi-asserted-by":"crossref","first-page":"653","DOI":"10.1140\/epjc\/s10052-021-09411-2","article-title":"The Higgs-portal for dark matter: Effective field theories versus concrete realizations","volume":"81","author":"Arcadi","year":"2021","journal-title":"Eur. Phys. J. C"},{"key":"ref_200","doi-asserted-by":"crossref","first-page":"080","DOI":"10.1007\/JHEP10(2020)080","article-title":"Pseudo-Goldstone dark matter: Gravitational waves and direct-detection blind spots","volume":"10","author":"Alanne","year":"2020","journal-title":"J. High Energy Phys."},{"key":"ref_201","doi-asserted-by":"crossref","first-page":"342","DOI":"10.1016\/j.physletb.2014.01.065","article-title":"The strangeness content of the nucleon from effective field theory and phenomenology","volume":"730","author":"Alarcon","year":"2014","journal-title":"Phys. Lett. B"},{"key":"ref_202","doi-asserted-by":"crossref","first-page":"138","DOI":"10.1007\/JHEP01(2019)138","article-title":"One-loop contribution to dark-matter-nucleon scattering in the pseudo-scalar dark matter model","volume":"1","author":"Azevedo","year":"2019","journal-title":"J. High Energy Phys."},{"key":"ref_203","doi-asserted-by":"crossref","first-page":"13","DOI":"10.1088\/0004-637X\/789\/1\/13","article-title":"Detection of An Unidentified Emission Line in the Stacked X-ray spectrum of Galaxy Clusters","volume":"789","author":"Bulbul","year":"2014","journal-title":"Astrophys. J."},{"key":"ref_204","doi-asserted-by":"crossref","first-page":"251301","DOI":"10.1103\/PhysRevLett.113.251301","article-title":"Unidentified Line in X-Ray Spectra of the Andromeda Galaxy and Perseus Galaxy Cluster","volume":"113","author":"Boyarsky","year":"2014","journal-title":"Phys. Rev. Lett."},{"key":"ref_205","doi-asserted-by":"crossref","first-page":"69","DOI":"10.1016\/j.physletb.2014.06.016","article-title":"The Poker Face of the Majoron Dark Matter Model: LUX to keV Line","volume":"735","author":"Queiroz","year":"2014","journal-title":"Phys. Lett. B"},{"key":"ref_206","unstructured":"Baek, S., Ko, P., and Park, W.I. (2014). The 3.5 keV X-ray line signature from annihilating and decaying dark matter in Weinberg model. arXiv."},{"key":"ref_207","doi-asserted-by":"crossref","first-page":"15","DOI":"10.1088\/1475-7516\/2014\/11\/015","article-title":"Decaying Vector Dark Matter as an Explanation for the 3.5 keV Line from Galaxy Clusters","volume":"11","author":"Farzan","year":"2014","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_208","doi-asserted-by":"crossref","first-page":"023","DOI":"10.1088\/1475-7516\/2015\/07\/023","article-title":"3.55 keV line in Minimal Decaying Dark Matter scenarios","volume":"7","author":"Arcadi","year":"2015","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"ref_209","doi-asserted-by":"crossref","first-page":"283","DOI":"10.1016\/j.physletb.2015.07.080","article-title":"Production of Sterile Neutrino Dark Matter and the 3.5 keV line","volume":"749","author":"Merle","year":"2015","journal-title":"Phys. Lett. B"},{"key":"ref_210","doi-asserted-by":"crossref","first-page":"095018","DOI":"10.1103\/PhysRevD.92.095018","article-title":"PeV neutrinos and a 3.5 keV x-ray line from a PeV-scale supersymmetric neutrino sector","volume":"92","author":"Roland","year":"2015","journal-title":"Phys. Rev. D"},{"key":"ref_211","doi-asserted-by":"crossref","first-page":"471","DOI":"10.1140\/epjc\/s10052-015-3702-4","article-title":"Upgrading sterile neutrino dark matter to FImP using scale invariance","volume":"75","author":"Kang","year":"2015","journal-title":"Eur. Phys. J. C"},{"key":"ref_212","doi-asserted-by":"crossref","first-page":"2435","DOI":"10.1088\/0264-9381\/23\/7\/014","article-title":"Detecting the cosmic gravitational wave background with the big bang observer","volume":"23","author":"Corbin","year":"2006","journal-title":"Class. Quant. Grav."},{"key":"ref_213","doi-asserted-by":"crossref","first-page":"221103","DOI":"10.1103\/PhysRevLett.87.221103","article-title":"Possibility of direct measurement of the acceleration of the universe using 0.1-Hz band laser interferometer gravitational wave antenna in space","volume":"87","author":"Seto","year":"2001","journal-title":"Phys. Rev. Lett."}],"container-title":["Symmetry"],"original-title":[],"language":"en","link":[{"URL":"https:\/\/www.mdpi.com\/2073-8994\/13\/10\/1945\/pdf","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2025,10,11]],"date-time":"2025-10-11T07:15:39Z","timestamp":1760166939000},"score":1,"resource":{"primary":{"URL":"https:\/\/www.mdpi.com\/2073-8994\/13\/10\/1945"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2021,10,15]]},"references-count":213,"journal-issue":{"issue":"10","published-online":{"date-parts":[[2021,10]]}},"alternative-id":["sym13101945"],"URL":"https:\/\/doi.org\/10.3390\/sym13101945","relation":{},"ISSN":["2073-8994"],"issn-type":[{"value":"2073-8994","type":"electronic"}],"subject":[],"published":{"date-parts":[[2021,10,15]]}}}