{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,9,17]],"date-time":"2026-09-17T04:05:06Z","timestamp":1789617906050,"version":"build-2803163510"},"reference-count":87,"publisher":"American Physical Society (APS)","issue":"13","license":[{"start":{"date-parts":[[2024,3,28]],"date-time":"2024-03-28T00:00:00Z","timestamp":1711584000000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"funder":[{"DOI":"10.13039\/501100002920","name":"Research Grants Council, University Grants Committee","doi-asserted-by":"publisher","award":["C6017-20G"],"award-info":[{"award-number":["C6017-20G"]}],"id":[{"id":"10.13039\/501100002920","id-type":"DOI","asserted-by":"publisher"}]},{"DOI":"10.13039\/501100011181","name":"Institute of High Energy Physics","doi-asserted-by":"publisher","award":["Y9291220K2"],"award-info":[{"award-number":["Y9291220K2"]}],"id":[{"id":"10.13039\/501100011181","id-type":"DOI","asserted-by":"publisher"}]}],"content-domain":{"domain":["journals.aps.org"],"crossmark-restriction":true},"short-container-title":["Phys. Rev. Lett."],"accepted":{"date-parts":[[2024,1,29]]},"abstract":"<jats:p>High-frequency gravitational waves (HFGWs) carry a wealth of information on the early Universe with a tiny comoving horizon and astronomical objects of small scale but with dense energy. We demonstrate that the nearby planets, such as Earth and Jupiter, can be utilized as a laboratory for detecting the HFGWs. These GWs are then expected to convert to signal photons in the planetary magnetosphere, across the frequency band of astronomical observation. As a proof of concept, we present the first limits from the existing low-Earth-orbit satellite for specific frequency bands and project the sensitivities for the future more-dedicated detections. The first limits from Juno, the latest mission orbiting Jupiter, are also presented. Attributed to the long path of effective GW-photon conversion and the wide angular distribution of signal flux, we find that these limits are highly encouraging, for a broad frequency range including a large portion unexplored before.<\/jats:p>\n                  <jats:sec>\n                    <jats:title\/>\n                    <jats:supplementary-material>\n                      <jats:permissions>\n                        <jats:copyright-statement>Published by the American Physical Society<\/jats:copyright-statement>\n                        <jats:copyright-year>2024<\/jats:copyright-year>\n                      <\/jats:permissions>\n                    <\/jats:supplementary-material>\n                  <\/jats:sec>","DOI":"10.1103\/physrevlett.132.131402","type":"journal-article","created":{"date-parts":[[2024,3,28]],"date-time":"2024-03-28T10:05:11Z","timestamp":1711620311000},"update-policy":"https:\/\/doi.org\/10.1103\/crossmark-policy","source":"Crossref","is-referenced-by-count":27,"title":["Limits on High-Frequency Gravitational Waves in Planetary Magnetospheres"],"prefix":"10.1103","volume":"132","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-5248-5076","authenticated-orcid":true,"given":"Tao","family":"Liu","sequence":"first","affiliation":[{"name":"Department of Physics and Jockey Club Institute for Advanced Study, The Hong Kong University of Science and Technology, Hong Kong S.A.R., People\u2019s Republic of China"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-2116-4659","authenticated-orcid":true,"given":"Jing","family":"Ren","sequence":"additional","affiliation":[{"name":"Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People\u2019s Republic of China"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-2650-6873","authenticated-orcid":true,"given":"Chen","family":"Zhang","sequence":"additional","affiliation":[{"name":"Department of Physics and Jockey Club Institute for Advanced Study, The Hong Kong University of Science and Technology, Hong Kong S.A.R., People\u2019s Republic of China"}],"role":[{"vocabulary":"crossref","role":"author"}]}],"member":"16","published-online":{"date-parts":[[2024,3,28]]},"reference":[{"key":"PhysRevLett.132.131402Cc1R1","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.116.061102"},{"key":"PhysRevLett.132.131402Cc2R1","doi-asserted-by":"publisher","DOI":"10.1007\/s41114-021-00032-5"},{"key":"PhysRevLett.132.131402Cc3R1","doi-asserted-by":"publisher","DOI":"10.1088\/0034-4885\/78\/12\/124901"},{"key":"PhysRevLett.132.131402Cc4R1","doi-asserted-by":"publisher","DOI":"10.1017\/pasa.2018.7"},{"key":"PhysRevLett.132.131402Cc5R1","doi-asserted-by":"publisher","DOI":"10.3390\/galaxies10010034"},{"key":"PhysRevLett.132.131402Cc6R1","first-page":"84","volume":"14","author":"M. 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