{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,7,3]],"date-time":"2025-07-03T04:18:28Z","timestamp":1751516308980,"version":"3.41.0"},"reference-count":19,"publisher":"Canadian Science Publishing","issue":"9","license":[{"start":{"date-parts":[[2015,9,1]],"date-time":"2015-09-01T00:00:00Z","timestamp":1441065600000},"content-version":"tdm","delay-in-days":0,"URL":"http:\/\/www.nrcresearchpress.com\/page\/about\/CorporateTextAndDataMining"}],"content-domain":{"domain":["cdnsciencepub.com"],"crossmark-restriction":false},"short-container-title":["Can. J. Phys."],"published-print":{"date-parts":[[2015,9]]},"abstract":"<jats:p> We derive the transformation properties of the internal energy and Kodama temperature of dynamical (spherically symmetric) black hole solutions generated through spacetime mappings. We use the Sultana-Dyer black hole and the Reissner\u2013Nordstr\u00f6m solution to provide prototypical examples testing our transformation formulae. <\/jats:p>","DOI":"10.1139\/cjp-2014-0487","type":"journal-article","created":{"date-parts":[[2015,1,22]],"date-time":"2015-01-22T22:36:50Z","timestamp":1421966210000},"page":"963-965","update-policy":"https:\/\/doi.org\/10.1139\/csp-crossmark-policy","source":"Crossref","is-referenced-by-count":0,"title":["Thermodynamics of apparent horizons under conformal and Kerr\u2013Schild maps"],"prefix":"10.1139","volume":"93","author":[{"given":"Valerio","family":"Faraoni","sequence":"first","affiliation":[{"name":"Physics Department, Bishop\u2019s University, 2600 College St., Sherbrooke, QC J1M 1Z7, Canada."}]},{"given":"Vincenzo","family":"Vitagliano","sequence":"additional","affiliation":[{"name":"CENTRA, Instituto Superior T\u00e9cnico, Universidade de Lisboa, Av. 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