Matches in SemOpenAlex for { <https://semopenalex.org/work/W3203325692> ?p ?o ?g. }
- W3203325692 abstract "A sensitive test for whether a black hole is a wormhole, using astronomical observations, would be to look for perturbations in the orbit of a pulsar around the black hole, caused by a perturbing object on the other side of the wormhole. By observing a pulsar in an orbit like that of S2 around the supermassive black hole at Sgr A* at the center of our Galaxy, the attainable mass limit on the perturber would be approximately ${10}^{4}$ times better than derived from current observations of S2. For a nominal stellar-mass black hole--pulsar binary, observing for 1 year could set a mass limit on a perturber more than 6 orders of magnitude better than for a pulsar orbiting Sgr A*. Observations of a star in a stellar-mass binary containing a black hole could set limits similar to the case of a pulsar orbiting Sgr A*." @default.
- W3203325692 created "2021-10-11" @default.
- W3203325692 creator A5004206059 @default.
- W3203325692 creator A5013651740 @default.
- W3203325692 creator A5032934538 @default.
- W3203325692 creator A5043097615 @default.
- W3203325692 creator A5078292842 @default.
- W3203325692 date "2021-10-06" @default.
- W3203325692 modified "2023-10-09" @default.
- W3203325692 title "Sensitive searches for wormholes" @default.
- W3203325692 cites W1498559808 @default.
- W3203325692 cites W1921030975 @default.
- W3203325692 cites W1974618482 @default.
- W3203325692 cites W1982501636 @default.
- W3203325692 cites W1986316936 @default.
- W3203325692 cites W1990678913 @default.
- W3203325692 cites W1993709057 @default.
- W3203325692 cites W2032573087 @default.
- W3203325692 cites W2050500992 @default.
- W3203325692 cites W2056598883 @default.
- W3203325692 cites W2069682152 @default.
- W3203325692 cites W2071342352 @default.
- W3203325692 cites W2082911982 @default.
- W3203325692 cites W2108025883 @default.
- W3203325692 cites W2125327258 @default.
- W3203325692 cites W2297596203 @default.
- W3203325692 cites W2416896665 @default.
- W3203325692 cites W2605004903 @default.
- W3203325692 cites W2733039922 @default.
- W3203325692 cites W2761455975 @default.
- W3203325692 cites W2895248736 @default.
- W3203325692 cites W2903375752 @default.
- W3203325692 cites W2908342113 @default.
- W3203325692 cites W2951829158 @default.
- W3203325692 cites W2978629607 @default.
- W3203325692 cites W2981054880 @default.
- W3203325692 cites W2994179738 @default.
- W3203325692 cites W2996071830 @default.
- W3203325692 cites W3002609495 @default.
- W3203325692 cites W3006864643 @default.
- W3203325692 cites W3023093278 @default.
- W3203325692 cites W3023522746 @default.
- W3203325692 cites W3041688503 @default.
- W3203325692 cites W3042619636 @default.
- W3203325692 cites W3045638888 @default.
- W3203325692 cites W3097320335 @default.
- W3203325692 cites W3098095284 @default.
- W3203325692 cites W3098357448 @default.
- W3203325692 cites W3098461838 @default.
- W3203325692 cites W3098820642 @default.
- W3203325692 cites W3099906373 @default.
- W3203325692 cites W3100799974 @default.
- W3203325692 cites W3100855252 @default.
- W3203325692 cites W3100928534 @default.
- W3203325692 cites W3101004335 @default.
- W3203325692 cites W3101308910 @default.
- W3203325692 cites W3101333992 @default.
- W3203325692 cites W3102218703 @default.
- W3203325692 cites W3102453565 @default.
- W3203325692 cites W3102689953 @default.
- W3203325692 cites W3103668758 @default.
- W3203325692 cites W3103705061 @default.
- W3203325692 cites W3104307500 @default.
- W3203325692 cites W3104409174 @default.
- W3203325692 cites W3105829920 @default.
- W3203325692 cites W3110185736 @default.
- W3203325692 cites W3119736528 @default.
- W3203325692 cites W3175446831 @default.
- W3203325692 cites W3195858618 @default.
- W3203325692 cites W4229824384 @default.
- W3203325692 cites W4231707210 @default.
- W3203325692 cites W4237837113 @default.
- W3203325692 cites W4288079901 @default.
- W3203325692 doi "https://doi.org/10.1103/physrevd.104.l081502" @default.
- W3203325692 hasPublicationYear "2021" @default.
- W3203325692 type Work @default.
- W3203325692 sameAs 3203325692 @default.
- W3203325692 citedByCount "23" @default.
- W3203325692 countsByYear W32033256922021 @default.
- W3203325692 countsByYear W32033256922022 @default.
- W3203325692 countsByYear W32033256922023 @default.
- W3203325692 crossrefType "journal-article" @default.
- W3203325692 hasAuthorship W3203325692A5004206059 @default.
- W3203325692 hasAuthorship W3203325692A5013651740 @default.
- W3203325692 hasAuthorship W3203325692A5032934538 @default.
- W3203325692 hasAuthorship W3203325692A5043097615 @default.
- W3203325692 hasAuthorship W3203325692A5078292842 @default.
- W3203325692 hasBestOaLocation W32033256921 @default.
- W3203325692 hasConcept C104954878 @default.
- W3203325692 hasConcept C105500671 @default.
- W3203325692 hasConcept C110363677 @default.
- W3203325692 hasConcept C121332964 @default.
- W3203325692 hasConcept C127413603 @default.
- W3203325692 hasConcept C1276947 @default.
- W3203325692 hasConcept C139153390 @default.
- W3203325692 hasConcept C146978453 @default.
- W3203325692 hasConcept C173120059 @default.
- W3203325692 hasConcept C18609725 @default.
- W3203325692 hasConcept C190330329 @default.
- W3203325692 hasConcept C196644772 @default.