Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-48282
Angélil, R; Saha, P (2011). Galactic-center S stars as a prospective test of the Einstein equivalence principle. Astrophysical Journal Letters, 734(1):L19.
View at publisher
The S stars in the Galactic-center region are found to be on near-perfect Keplerian orbits around presumably a supermassive black hole, with periods of 15-50 yr. Since these stars reach a few percent of light speed at pericenter, various relativistic effects are expected and have been discussed in the literature. We argue that an elegant test of the Einstein equivalence principle should be possible with existing instruments, through spectroscopic monitoring of an S star concentrated during the months around pericenter, supplemented with an already-adequate astrometric determination of the inclination. In essence, the spectrum of an S star can be considered a heterogeneous ensemble of clocks in a freely falling frame, which near pericenter is moving at relativistic speeds.
16 downloads since deposited on 18 Feb 2012
2 downloads since 12 months
|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Dewey Decimal Classification:||530 Physics|
|Deposited On:||18 Feb 2012 14:17|
|Last Modified:||14 Feb 2014 20:05|
|Publisher:||Institute of Physics Publishing|
|ISSN:||0004-637X (P) 1538-4357 (E)|
Users (please log in): suggest update or correction for this item
Repository Staff Only: item control page