期刊
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
卷 -, 期 3, 页码 -出版社
IOP Publishing Ltd
DOI: 10.1088/1475-7516/2022/03/007
关键词
GR black holes; Wormholes; gravity
资金
- Consejeria de Educacion de la Junta de Castilla y Leon
- Fondo Social Europeo
- Ayuda [IJCI2018-036198-I, MCIN/AEI/10.13039/501100011033]
- FSE El FSE invierte en tu futuro o Financiado por la Union Europea NextGenerationEU/PRTR [PGC2018-096038-B-I00]
- Spanish Ministerio de Ciencia e Innovacion
- FEDER A way of making Europe [SA096P20]
- Junta de Castilla y Leon
Despite the improvements in future observations, it remains difficult to determine whether the central supermassive object is a black hole or a wormhole. The study used data from the S0-2 star and simulated observations to investigate the nature of the object, but was unable to definitively distinguish between the two possibilities. However, it was found that stars orbiting closer to the object could provide valuable insights into its fundamental nature.
Despite the huge improvements guaranteed by future GRAVITY observations of the S0-2 star, these will not be able to unveil the fundamental nature, whether black hole or wormhole, of the central supermassive object. Nevertheless, observing stars orbiting closer to the central gravitational source could allow to distinguish between the black hole and wormhole nature of this object at more than 5 sigma. Firstly, we have used publicly available astrometric and spectroscopic measurements of the S0-2 star to constrain the metric around the supermassive object without finding any evidence either favouring or ruling out the wormhole nature. Secondly, we have designed a mock catalogue of future observations of the S0-2 star mirroring the accuracy and precision of GRAVITY. Afterwards, we firstly tested our methodology showing that our procedure recovers the input model, and subsequently we demonstrated that the constraining power of such a dataset is not enough to distinguish between black hole and wormhole. Finally, we built some toy models representing stars orbiting much closer the central object than S0-2. We used these toy models to investigate which are the ideal orbital features and observational strategies to achieve our aim of unveiling the fundamental nature of the central supermassive object, demonstrating that a star with a period of the order of similar to 5 years and a pericentre distance of similar to 5 AU could identify the nature of the central object at almost 5 sigma accuracy.
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