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Expansion-induced contribution to the precession of binary orbits

Brett Bolen, Luca Bombelli and Raymond Puzio

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We point out the existence of new effects of global spacetime expansion on local binary systems. In addition to a possible change of orbital size, there is a contribution to the precession of elliptic orbits, to be added to the well known general relativistic effect in static spacetimes, and the eccentricity can change. Our model calculations are done using geodesics in a McVittie metric, representing a localized system in an asymptotically Robertson-Walker spacetime; we give a few numerical estimates for that case, and briefly comment on ways in which the model should be improved.


PACS

04.25.-g Approximation methods; equations of motion

04.20.-q Classical general relativity

98.80.Es Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc)

95.30.Sf Relativity and gravitation

98.80.Jk Mathematical and relativistic aspects of cosmology

MSC

83C05 Einstein's equations (general structure, canonical formalism, Cauchy problems)

83F05 Cosmology

83C25 Approximation procedures, weak fields

Subjects

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 7 (7 April 2001)

Received 11 December 2000



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