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Issue Date
Title
Author(s)
Citation
Nov-2007
Higher signal harmonics, LISA's angular resolution, and dark energy
Arun, K.G.
;
Iyer, B.R.
;
Sathyaprakash, B.S.
;
Sinha, Siddhartha
;
Van den Broeck, Chris
Physical Review D, 2007, Vol.76, p104016-1
25-Oct-2000
Book review of “Computational physics: An introduction” by R. C. Verma, et al.
Iyer, B.R.
;
Madhusudana, H.R.
Current Science, 2000, Vol. 79, p1113-1114.
6-Jan-2005
Hadamard regularization of the third post-Newtonian gravitational wave generation of two point masses
Blanchet, Luc
;
Iyer, B.R.
Physical Review D, 2005, Vol.71, 024004
26-Aug-2004
Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order
Blanchet, Luc
;
Damour, Thibault
;
Esposito-Farese, G.
;
Iyer, B.R.
Physical Review Letters, 2004, Vol.93, 091101
17-Sep-2004
Phasing of gravitational waves from inspiralling eccentric binaries
Damour, Thibault
;
Gopakumar, A.
;
Iyer, B.R.
Physical Review D, 2004, Vol.70, 064028
2002
Gravitational wave astronomy: Probing physics and unravelling astrophysics
Iyer, B.R.
Bulletin of the Astronomical Society of India, 2002, Vol.30, p735-740
25-Feb-2005
New class of post-Newtonian approximants to the waveform templates of inspiralling compact binaries: Test mass in the Schwarzschild spacetime
Ajith, P.
;
Iyer, B.R.
;
Robinson, C.A.K.
;
Sathyaprakash, B.S.
Physical Review D, 2005, Vol.71, 044029
15-Mar-2002
Gravitational-wave inspiral of compact binary systems to 7/2 post-Newtonian order
Blanchet, Luc
;
Guillaume, Faye
;
Iyer, B.R.
;
Joguet, Benoit
http://prola.aps.org/abstract/PRD/v65/i6/e061501
15-Aug-2000
Padé approximants for truncated post-Newtonian neutron star models
Gupta, Anshu
;
Gopakumar, A.
;
Iyer, B.R.
;
Iyer, Sai
Physical Review D, 2000, Vol.62, 044038
9-May-2006
Testing post-Newtonian theory with gravitational wave observations
Arun, K.G.
;
Iyer, B.R.
;
Qusailah, M.S.S.
;
Sathyaprakash, B.S.
Classical and Quantum Gravity, 2006, Vol.23 pL37-L43
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13
Blanchet, Luc
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Arun, K.G.
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5
Gopakumar, A.
5
Qusailah, M.S.S.
2
Ajith, P.
2
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.
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