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<title>Unveiling the nature of SgrA* with the geodesic motion of S-stars</title>
<creator>Monica, Riccardo della</creator>
<creator>Martino, Iván de</creator>
<subject>Agujeros negros</subject>
<subject>Agujeros de gusanos</subject>
<subject>GR black holes</subject>
<subject>Wormholes</subject>
<subject>Gravity</subject>
<description>[EN]Despite the huge improvements guaranteed by future GRAVITY observations of&#xd;
the S0-2 star, these will not be able to unveil the fundamental nature, whether black hole or&#xd;
wormhole, of the central supermassive object. Nevertheless, observing stars orbiting closer&#xd;
to the central gravitational source could allow to distinguish between the black hole and&#xd;
wormhole nature of this object at more than 5 .&#xd;
Firstly, we have used publicly available astrometric and spectroscopic measurements of&#xd;
the S0-2 star to constrain the metric around the supermassive object without finding any&#xd;
evidence either favouring or ruling out the wormhole nature. Secondly, we have designed a&#xd;
mock catalogue of future observations of the S0-2 star mirroring the accuracy and precision&#xd;
of GRAVITY. Afterwards, we firstly tested our methodology showing that our procedure&#xd;
recovers the input model, and subsequently we demonstrated that the constraining power of&#xd;
such a dataset is not enough to distinguish between black hole and wormhole. Finally, we&#xd;
built some toy models representing stars orbiting much closer the central object than S0-2.&#xd;
We used these toy models to investigate which are the ideal orbital features and observational&#xd;
strategies to achieve our aim of unveiling the fundamental nature of the central supermassive&#xd;
object, demonstrating that a star with a period of the order of   5 years and a pericentre&#xd;
distance of   5AU could identify the nature of the central object at almost 5  accuracy.</description>
<date>2025-01-09</date>
<date>2025-01-09</date>
<date>2022-03</date>
<type>info:eu-repo/semantics/article</type>
<identifier>Riccardo Della Monica and Ivan de Martino JCAP03(2022)007</identifier>
<identifier>1475-7516</identifier>
<identifier>http://hdl.handle.net/10366/161446</identifier>
<identifier>10.1088/1475-7516/2022/03/007</identifier>
<identifier>1475-7516</identifier>
<language>eng</language>
<relation>https://dx.doi.org/10.1088/1475-7516/2022/03/007</relation>
<relation>IJCI2018-036198-I</relation>
<relation>PGC2018- 096038-B-I00</relation>
<rights>info:eu-repo/semantics/openAccess</rights>
<publisher>IOP Publishing</publisher>
</thesis></metadata></record></GetRecord></OAI-PMH>