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Employing the two-fluid formalism, our analysis reveals that DM accrued within the NS core exerts an inward gravitational pull on the outer layers composed of BM. This gravitational interaction results in a noticeable increase in baryonic density within the core of the NS. Consequently, it strongly affects the star\u2019s thermal evolution by triggering the early onsets of the direct Urca (DU) processes, causing enhanced neutrino emission and rapid star cooling. Moreover, the photon emission from the star\u2019s surface is modified due to a reduction in radius. We demonstrate the effect of DM gravitational pull on nucleonic and hyperonic DU processes that become kinematically allowed even for NSs of low mass. We then discuss the significance of observing NSs at various distances from the Galactic center. Given that the DM distribution peaks toward the Galactic center, NSs within this central region are expected to harbor higher fractions of DM, potentially leading to distinct cooling behaviors.<\/jats:p>","DOI":"10.3390\/particles7010010","type":"journal-article","created":{"date-parts":[[2024,2,28]],"date-time":"2024-02-28T07:56:02Z","timestamp":1709106962000},"page":"179-200","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":15,"title":["The Impact of Asymmetric Dark Matter on the Thermal Evolution of Nucleonic and Hyperonic Compact Stars"],"prefix":"10.3390","volume":"7","author":[{"ORCID":"https:\/\/orcid.org\/0000-0001-9545-466X","authenticated-orcid":false,"given":"Edoardo","family":"Giangrandi","sequence":"first","affiliation":[{"name":"CFisUC, Department of Physics, University of Coimbra, Rua Larga, 3004-516 Coimbra, Portugal"},{"name":"Institut f\u00fcr Physik und Astronomie, Universit\u00e4t Potsdam, Karl-Liebknecht-Str. 24-25, 14476 Potsdam, Germany"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-8880-039X","authenticated-orcid":false,"given":"Afonso","family":"\u00c1vila","sequence":"additional","affiliation":[{"name":"CFisUC, Department of Physics, University of Coimbra, Rua Larga, 3004-516 Coimbra, Portugal"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-5854-1617","authenticated-orcid":false,"given":"Violetta","family":"Sagun","sequence":"additional","affiliation":[{"name":"CFisUC, Department of Physics, University of Coimbra, Rua Larga, 3004-516 Coimbra, Portugal"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-4947-8721","authenticated-orcid":false,"given":"Oleksii","family":"Ivanytskyi","sequence":"additional","affiliation":[{"name":"Incubator of Scientific Excellence\u2014Centre for Simulations of Superdense Fluids, University of Wroc\u0142aw, 50-204 Wroclaw, Poland"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-6464-8023","authenticated-orcid":false,"given":"Constan\u00e7a","family":"Provid\u00eancia","sequence":"additional","affiliation":[{"name":"CFisUC, Department of Physics, University of Coimbra, Rua Larga, 3004-516 Coimbra, Portugal"}]}],"member":"1968","published-online":{"date-parts":[[2024,2,27]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","unstructured":"Baym, G., Hatsuda, T., Kojo, T., Powell, P.D., Song, Y., and Takatsuka, T. 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