Magnetized Accretion onto Inspiraling Binary Black Holes - LUTH
Magnetized Accretion onto Inspiraling Binary Black Holes - LUTH
Magnetized Accretion onto Inspiraling Binary Black Holes - LUTH
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Ricci Scalar: Case for Higher Order Approximations.<br />
2nd: 4th:<br />
Rtt = 0.01024587050684905 Rtt = 0.01007850127240062<br />
Rtx = 0.03228380078907006 Rtx = 0.0340889478274195<br />
Rty = −0.02308902839605859 Rty = −0.02298639795941293<br />
Rtz = −0.02006201110556877 Rtz = −0.02032786334618492<br />
Rxx = −0.6774182693609987 Rxx = −0.6650699268486431<br />
Rxy = 0.3413360547161979 Rxy = 0.3261324979719031<br />
Rxz = 0.348427534006535 Rxz = 0.3356062612167152<br />
Ryy = −0.1977530448946112 Ryy = −0.2060409626394311<br />
Ryz = −0.1865524325067573 Ryz = −0.1884958238515893<br />
Rzz = −0.2906179378901275 Rzz = −0.297516599915685<br />
R = −0.2657411795293186 R = −0.2698938651121096<br />
H = 0.01469997464077989 H = 0.0131591785513933<br />
M = 0.01504264551925634 M = 0.0167759321900986<br />
Table: Ricci tensor, scalar and constraints calculated using 2nd (left) and 4th<br />
(right) order FDA operators.<br />
Bruno C. Mundim <strong>Magnetized</strong> <strong>Accretion</strong> <strong>onto</strong> <strong>Inspiraling</strong> BBH 2013-05-23
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