Gravitational Waves from Inspiralling Compact Binaries in ... - LUTH
Gravitational Waves from Inspiralling Compact Binaries in ... - LUTH Gravitational Waves from Inspiralling Compact Binaries in ... - LUTH
3PN accurate conservative dynamics The angular motion, described in terms of φ and ˙ φ, is given by φ(λ, l) = λ + W (l) , λ = (1 + k)l , k = 3ξ2/3 1 − e2 ξ + t 4/3 4(1 − e2 t )2 2 78 − 28η + (51 − 26η)et + ξ2 128(1 − e2 t )3 18240 − 25376η + 492π 2 η + 896η 2 + (28128 − 27840η + 123π 2 η + 5120η 2 )e 2 t + (2496 − 1760η + 1040η 2 )e 4 t + 1920 − 768η + (3840 − 1536η)e 2 t 1 − e2 t , W (l) = WN + W1PN + W2PN + W3PN , WN = v − u + et sin u , W1PN = 3ξ2/3 1 − e 2 t (v − u + et sin u) , BRI-IHP06-I – p.122/??
3PN accurate conservative dynamics W2PN = + W3PN = ξ 4/3 32(1 − e 2 t )2 (1 − et cos u) 3 × 8 78 − 28η + (51 − 26η)e 2 t − 6(5 − 2η)(1 − e 2 t ) 3/2 (v − u)(1 − et cos u) 3 624 − 284η + 4η 2 + (408 − 88η − 8η 2 )e 2 t − (60η − 4η 2 )e 4 t + et cos u − 1872 + 792η − 8η 2 − (1224 − 384η − 16η 2 )e 2 t + (120η − 8η 2 )e 4 t + 1872 − 732η + 4η 2 + (1224 − 504η − 8η 2 )e 2 t − (60η − 4η2 )e 4 t (et cos u) 2 + −624 + 224η − (408 − 208η)e 2 t (et cos u) 3 et sin u + − (8 + 153η − 27η 2 )e 2 t + (4η − 12η2 )e 4 t + 8 + 152η − 24η 2 + (8 + 146η − 6η 2 ) ×et cos u + −8 − 148η + 12η 2 − (η − 3η 2 )e 2 t ξ 2 (1 − e 2 t )3 (1 − et cos u) 5 · · · · · · · , × (et cos u) 2 et sin u 1 − e2 t BRI-IHP06-I – p.123/??
- Page 73 and 74: Far Zone Angular Momentum Flux dJi
- Page 75 and 76: 3PN AMFlux - Shar dJi dt dJi dt
- Page 77 and 78: Orbital Averaged AMF - ADM Using th
- Page 79 and 80: Orbital Averaged AMF - ADM 〈 dJ d
- Page 81 and 82: Orbital Averaged AMF - ADM 〈 dJ d
- Page 83 and 84: Evoln of orbital elements under GRR
- Page 85 and 86: Evoln of orbital element n under GR
- Page 87 and 88: Evoln of orbital element n under GR
- Page 89 and 90: Evoln of orbital element et under G
- Page 91 and 92: Evoln of orbital element ar under G
- Page 93 and 94: Evoln of orbital element ar under G
- Page 95 and 96: PART II Based on Phasing of Gravita
- Page 97 and 98: Beyond Orbital Averages Going beyon
- Page 99 and 100: Phasing of GWF TT radn field is giv
- Page 101 and 102: Phasing of GWF Orbital phase = φ,
- Page 103 and 104: Method of variation of constants A
- Page 105 and 106: Method of variation of constants c1
- Page 107 and 108: Method of variation of constants At
- Page 109 and 110: Method of variation of constants An
- Page 111 and 112: Method of variation of constants Al
- Page 113 and 114: Method of variation of constants Fo
- Page 115 and 116: Method of variation of constants Du
- Page 117 and 118: Implementation Compute 3PN accurate
- Page 119 and 120: 3PN accurate conservative dynamics
- Page 121 and 122: 3PN accurate conservative dynamics
- Page 123: 3PN accurate conservative dynamics
- Page 127 and 128: 3PN accurate conservative dynamics
- Page 129 and 130: 3.5PN accurate reactive dynamics A
- Page 131 and 132: 3.5PN accurate reactive dynamics Fi
- Page 133 and 134: 3.5PN accurate reactive dynamics dc
- Page 135 and 136: 3.5PN accurate reactive dynamics 4
- Page 137 and 138: Secular variations d¯n dt dēt dt
- Page 139 and 140: Periodic variations To complete thi
- Page 141 and 142: Periodic variations One can analyti
- Page 143 and 144: Periodic variations ˜cl = − 2ξ5
- Page 145 and 146: Periodic variations Above results m
- Page 147 and 148: Periodic variations ˜ l(l; ¯ca) =
- Page 149 and 150: ¯n/ni and ñ/n versus l/(2π) n /
- Page 151 and 152: h+(t) and h×(t) Scaled h + (t) Sca
- Page 153 and 154: ¯n/ni and ñ/n ēt and ˜et versus
- Page 155 and 156: ¯cl and ˜cl ¯cλ and ˜cλ versu
- Page 157 and 158: Validity of Results Circular orbits
- Page 159: References 1. P. C. Peters, Phys. R
3PN accurate conservative dynamics<br />
W2PN =<br />
+<br />
W3PN =<br />
ξ 4/3<br />
32(1 − e 2 t )2 (1 − et cos u) 3<br />
×<br />
<br />
8 78 − 28η + (51 − 26η)e 2 t − 6(5 − 2η)(1 − e 2 t ) 3/2 (v − u)(1 − et cos u) 3<br />
<br />
624 − 284η + 4η 2 + (408 − 88η − 8η 2 )e 2 t − (60η − 4η 2 )e 4 t +<br />
et cos u<br />
− 1872 + 792η − 8η 2 − (1224 − 384η − 16η 2 )e 2 t + (120η − 8η 2 )e 4 t<br />
+ 1872 − 732η + 4η 2 + (1224 − 504η − 8η 2 )e 2 t − (60η − 4η2 )e 4 <br />
t (et cos u) 2<br />
+ −624 + 224η − (408 − 208η)e 2 <br />
t (et cos u) 3<br />
<br />
et s<strong>in</strong> u +<br />
<br />
− (8 + 153η − 27η 2 )e 2 t + (4η − 12η2 )e 4 t + 8 + 152η − 24η 2 + (8 + 146η − 6η 2 )<br />
×et cos u + −8 − 148η + 12η 2 − (η − 3η 2 )e 2 t<br />
ξ 2<br />
(1 − e 2 t )3 (1 − et cos u) 5<br />
<br />
· · · · · · ·<br />
<br />
,<br />
<br />
× (et cos u) 2<br />
<br />
et s<strong>in</strong> u 1 − e2 t<br />
BRI-IHP06-I – p.123/??