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scoap3/articles/tests/data/record_failing_on_airflow.json
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{ | ||
"dois":[ | ||
{ | ||
"value":"10.1103/PhysRevD.109.046003" | ||
} | ||
], | ||
"page_nr":[ | ||
17 | ||
], | ||
"arxiv_eprints":[ | ||
{ | ||
"value":"2312.06750", | ||
"categories":[ | ||
"hep-th", | ||
"gr-qc", | ||
"math-ph", | ||
"math.MP" | ||
] | ||
} | ||
], | ||
"authors":[ | ||
{ | ||
"full_name":"Chatwin-Davies, Aidan", | ||
"given_names":"Aidan", | ||
"surname":"Chatwin-Davies", | ||
"affiliations":[ | ||
{ | ||
"value":"Okinawa Institute of Science and Technology, 1919-1 Tancha, Onna-son, Kunigami-gun, Okinawa, 904-0495, Japan", | ||
"organization":"Okinawa Institute of Science and Technology, 1919-1 Tancha, Onna-son, Kunigami-gun, Okinawa, 904-0495", | ||
"country":"Japan" | ||
} | ||
] | ||
}, | ||
{ | ||
"full_name":"Leung, Pompey", | ||
"given_names":"Pompey", | ||
"surname":"Leung", | ||
"affiliations":[ | ||
{ | ||
"value":"Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, V6T 1Z1, Canada", | ||
"organization":"Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, V6T 1Z1", | ||
"country":"Canada" | ||
} | ||
] | ||
}, | ||
{ | ||
"full_name":"Remmen, Grant N.", | ||
"given_names":"Grant N.", | ||
"surname":"Remmen", | ||
"affiliations":[ | ||
{ | ||
"value":"Center for Cosmology and Particle Physics, Department of Physics, New York University, New York, New York, 10003, USA", | ||
"organization":"Center for Cosmology and Particle Physics, Department of Physics, New York University, New York, New York, 10003", | ||
"country":"USA" | ||
} | ||
] | ||
} | ||
], | ||
"license":[ | ||
{ | ||
"url":"https://creativecommons.org/licenses/by/4.0/", | ||
"license":"CC-BY-4.0" | ||
} | ||
], | ||
"collections":[ | ||
{ | ||
"primary":"HEP" | ||
}, | ||
{ | ||
"primary":"Citeable" | ||
}, | ||
{ | ||
"primary":"Published" | ||
} | ||
], | ||
"publication_info":[ | ||
{ | ||
"journal_title":"Physical Review D", | ||
"journal_volume":"109", | ||
"year":2024, | ||
"journal_issue":"4", | ||
"material":"article" | ||
} | ||
], | ||
"abstracts":[ | ||
{ | ||
"value":"<p>Holographic screens are codimension-one hypersurfaces that extend the notion of apparent horizons to general (non-black hole) spacetimes and that display interesting thermodynamic properties. We show that if a spacetime contains a codimension-two, boundary-homologous, minimal extremal spacelike surface <math xmlns=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mi>X</mi></math> (known as an HRT surface in <math xmlns=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mrow><mi>AdS</mi><mo>/</mo><mi>CFT</mi></mrow></math>), then any holographic screens are sequestered to the causal wedges of <math xmlns=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mi>X</mi></math>. That is, any single connected component of a holographic screen can be located in at most one of the causal future, causal past, inner wedge, or outer wedge of <math xmlns=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mi>X</mi></math>. We comment on how this result informs possible coarse grained entropic interpretations of generic holographic screens, as well as on connections to semiclassical objects such as quantum extremal surfaces.</p>", | ||
"source":"APS" | ||
} | ||
], | ||
"acquisition_source":{ | ||
"source":"APS", | ||
"method":"APS", | ||
"date":"2024-02-08T00:00:16.954712" | ||
}, | ||
"copyright":[ | ||
{ | ||
"year":2024, | ||
"statement":"Published by the American Physical Society" | ||
} | ||
], | ||
"imprints":[ | ||
{ | ||
"date":"2024-02-07", | ||
"publisher":"APS" | ||
} | ||
], | ||
"record_creation_date":"2024-02-08T00:00:16.954712", | ||
"titles":[ | ||
{ | ||
"title":"Holographic screen sequestration", | ||
"source":"APS" | ||
} | ||
], | ||
"$schema":"https://repo.qa.scoap3.org/schemas/hep.json" | ||
} |
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