{"paper":{"title":"Dense matter with eXTP","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Achim Schwenk, Aleksi Kurkela, Alessandro Patruno, Alessandro Riggio, Alexander Heger, Altan Baykal, Andrea Possenti, Andrea Sanna, Andrea Santangelo, Andrea Vacchi, Angelo F. Gambino, Ang Li, Anna L. Watts, Benjamin Stappers, Can Gungor, Chanda Prescod-Weinstein, David Tsang, Deepto Chakrabarty, Dieter H. Hartmann, Edward Brown, Eva \\v{S}r\\'amkov\\'a, Fangjun Lu, Federico Bernardini, Gabriel T\\\"or\\\"ok, Guobao Zhang, Hendrik Schatz, Holger Stiele, Ignazio Bombaci, Ingo Tews, Jean in 't Zand, Jeroen Homan, J\\'er\\^ome Chenevez, JinLu Qu, Joonas N\\\"attil\\\"a, Juri Poutanen, Kai Hebeler, Laura Tolos, Liming Song, Long Ji, Manuel Linares, Marco Feroci, Mariano M\\'endez, Martin Urbanec, Maurizio Falanga, M. Coleman Miller, Melania Del Santo, Mingyu Ge, Nathalie Degenaar, Oleg Kargaltsev, Pavel Bakala, Renxin Xu, Robert D. Ferdman, Rosario Iaria, Sebastien Guillot, Sharon Morsink, Shijie Zheng, ShuangNan Zhang, Shu Zhang, Silvia Zane, Simin Mahmoodifar, Slavko Bogdanov, Sudip Bhattacharyya, Svenja K. Greif, Thomas E. Riley, Tiziana Di Salvo, Tod Strohmayer, Tuomo Salmi, Victor Doroshenko, Wenda Zhang, Wenfei Yu, Xiangdong Li, Xiaoyu Lai, Xia Zhou, Ypeng Xu, Yuri Cavecchi, Zhaosheng Li","submitted_at":"2018-12-10T19:00:41Z","abstract_excerpt":"In this White Paper we present the potential of the Enhanced X-ray Timing and Polarimetry (eXTP) mission for determining the nature of dense matter; neutron star cores host an extreme density regime which cannot be replicated in a terrestrial laboratory. The tightest statistical constraints on the dense matter equation of state will come from pulse profile modelling of accretion-powered pulsars, burst oscillation sources, and rotation-powered pulsars. Additional constraints will derive from spin measurements, burst spectra, and properties of the accretion flows in the vicinity of the neutron s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.04021","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}