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Browsing by Author "Iyer, B.R."

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Issue DateTitleAuthor(s)Citation
9-Mar-1978 Spontaneous creation of massive spin half particles by a rotating black holeIyer, B.R.; Kumar, ArvindPramana, 1978, Vol.1, p171
May-2008 Summary of session B3: analytic approximations, perturbation methods and their applicationsJaranowski, P.; Arun, K.G.; Iyer, B.R.; and 22 co-authorsClassical and Quantum Gravity, 2008, Vol.25, 114020
7-Jan-2005 Surface-integral expressions for the multipole moments of post-Newtonian sources and the boosted Schwarzschild solutionBlanchet, Luc; Damour, Thibault; Iyer, B.R.Classical and Quantum Gravity, 2005, Vol.22, p155-181
Mar-2008 Tail effects in the third post-Newtonian gravitational wave energy flux of compact binaries in quasi-elliptical orbitsArun, K.G.; Blanchet, Luc; Iyer, B.R.; Qusailah, M.S.S.Physical Review D, 2008, Vol.77, 064034
9-May-2006 Testing post-Newtonian theory with gravitational wave observationsArun, K.G.; Iyer, B.R.; Qusailah, M.S.S.; Sathyaprakash, B.S.Classical and Quantum Gravity, 2006, Vol.23 pL37-L43
11-Dec-2009 Third post-Newtonian angular momentum flux and the secular evolution of orbital elements for inspiralling compact binaries in quasi-elliptical orbitsArun, K.G.; Blanchet, Luc; Iyer, B.R.; Sinha, SiddharthaPhysical Review D, 2009, Vol.80, p124018
Feb-2003 Third post-Newtonian dynamics of compact binaries: equations of motion in the centre-of-mass frameBlanchet, Luc; Iyer, B.R.Classical and Quantum Gravity, 2003, Vol.20, p755-776
Jul-2008 The third post-Newtonian gravitational wave polarizations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbitsBlanchet, Luc; Faye, Guillaume; Iyer, B.R.; Sinha, SiddharthaClassical and Quantum Gravity, 2008, Vol.25, 165003
Mar-1985 Ultracompact (R<3 M) objects in general relativityIyer, B.R.; Vishveshwara, C.V.; Dhurandhar, S.V.Classical and Quantum Gravity, 1985, Vol.2, p219-228
Jun-1989 The Vaidya solution in higher dimensionsIyer, B.R.; Vishveshwara, C.V.Pramana, 1989, Vol. 32, p749-752.
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