000126615 001__ 126615 000126615 005__ 20240731103419.0 000126615 0247_ $$2doi$$a10.1088/1742-6596/2502/1/012004 000126615 0248_ $$2sideral$$a134083 000126615 037__ $$aART-2023-134083 000126615 041__ $$aeng 000126615 100__ $$0(orcid)0000-0002-6948-5101$$aCebrián, Susana$$uUniversidad de Zaragoza 000126615 245__ $$aReview on dark matter searches 000126615 260__ $$c2023 000126615 5060_ $$aAccess copy available to the general public$$fUnrestricted 000126615 5203_ $$aDark matter particles populating our galactic halo could be directly detected by measuring their scattering off target nuclei or electrons in a suitable detector. As this interaction is expected to occur with very low probability and would generate very small energy deposits, the detection is challenging; the possible identification of distinctive signatures (like an annual modulation in the interaction rates or directionality) to assign a dark matter origin to a possible observation is being considered. Here, the physics case of different dark matter direct detection experiments will be presented and the different and complementary techniques which are being applied or considered will be discussed, summarizing their features and latest results obtained. Special focus will be made on TPC-related projects; experiments using noble liquids have presently a leading role to constrain interaction cross sections of a wide range of dark matter candidates and gaseous detectors are very promising to explore specifically low mass dark matter as well as to measure directionality. 000126615 540__ $$9info:eu-repo/semantics/openAccess$$aby$$uhttp://creativecommons.org/licenses/by/3.0/es/ 000126615 592__ $$a0.18$$b2023 000126615 593__ $$aPhysics and Astronomy (miscellaneous)$$c2023 000126615 594__ $$a1.2$$b2023 000126615 655_4 $$ainfo:eu-repo/semantics/conferenceObject$$vinfo:eu-repo/semantics/publishedVersion 000126615 7102_ $$12004$$2390$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Física Atóm.Molec.y Nucl. 000126615 773__ $$g2502, 1 (2023), 012004 [12 pp.]$$pJ. Phys.: Conf. Ser.$$tJournal of Physics: Conference Series$$x1742-6588 000126615 8564_ $$s532338$$uhttps://zaguan.unizar.es/record/126615/files/texto_completo.pdf$$yVersión publicada 000126615 8564_ $$s2217318$$uhttps://zaguan.unizar.es/record/126615/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada 000126615 909CO $$ooai:zaguan.unizar.es:126615$$particulos$$pdriver 000126615 951__ $$a2024-07-31-10:08:41 000126615 980__ $$aARTICLE