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from math import pi as PI | ||
from math import log, fabs, sqrt | ||
from numba import vectorize, cuda | ||
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from math import pi as PI | ||
from math import log, fabs, sqrt | ||
GAMMA = 0.5772156649015329 | ||
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@cuda.jit(device=True) | ||
def TaylorT3_Omega_new(t, tc, eta, M): | ||
Msec = M | ||
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pi2 = PI*PI | ||
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c1 = eta/(5.*Msec) | ||
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td = c1 * (tc - t) | ||
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theta = td**(-1./8.) | ||
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theta2 = theta*theta | ||
theta3 = theta2*theta | ||
theta4 = theta3*theta | ||
theta5 = theta4*theta | ||
theta6 = theta5*theta | ||
theta7 = theta6*theta | ||
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# pre factor | ||
ftaN = 1. / ( 8. * PI * Msec ) | ||
# 0PN | ||
fts1 = 1. | ||
# 0.5PN = 0 in GR | ||
# 1PN | ||
fta2 = 7.43/26.88 + 1.1/3.2 * eta | ||
# 1.5PN | ||
fta3 = -3./10. * PI | ||
# 2PN | ||
fta4 = 1.855099/14.450688 + 5.6975/25.8048 * eta + 3.71/20.48 * eta*eta | ||
# 2.5PN | ||
fta5 = (-7.729/21.504 + 1.3/25.6 * eta) * PI | ||
# 3PN | ||
fta6 = -7.20817631400877/2.88412611379200 + 5.3/20.0 * pi2 + 1.07/2.80 * GAMMA \ | ||
+ (25.302017977/4.161798144 - 4.51/20.48 * pi2) * eta \ | ||
- 3.0913/183.5008 * eta*eta + 2.35925/17.69472 * eta*eta*eta | ||
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# 3.5PN | ||
fta7 = (-1.88516689/4.33520640 - 9.7765/25.8048 * eta + 1.41769/12.90240 * eta*eta) * PI | ||
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# 3PN log term | ||
ftal6 = 1.07/2.80 | ||
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full = theta3*ftaN * (fts1 \ | ||
+ fta2*theta2 \ | ||
+ fta3*theta3 \ | ||
+ fta4*theta4 \ | ||
+ fta5*theta5 \ | ||
+ (fta6 + ftal6*log(2.*theta))*theta6 \ | ||
+ fta7*theta7) | ||
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return full * 2 * PI # 2pi to go from freq to angular freq | ||
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@cuda.jit(device=True) | ||
def freq_ins_ansatz(t, eta, tc,b,c,M): | ||
""" | ||
this is the frequency inspiral ansatz. | ||
I needed an separate function so that I could use it in the amplitude inspiral model | ||
""" | ||
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tau = eta * (tc - t) / (5*M) | ||
model = TaylorT3_Omega_new(t, tc, eta, M) + b*tau**(-9./8.) + c*tau**(-10./8.) | ||
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return model | ||
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@cuda.jit(device=True) | ||
def Hhat22_x(x, eta): | ||
C = 0.577216 # is the Euler constant | ||
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xarr0 = 1. | ||
xarr1 = -107./42 + 55*eta/42 | ||
xarr2 = 2.*PI | ||
xarr3 = -2173./1512 - 1069.*eta/216 + 2047.*eta**2/1512 | ||
xarr4 = (-107*PI/21 - 24.*1.j*eta + 34.*PI*eta/21) | ||
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x5a = 27027409./646800 - 856.*C/105 + 428*1.j*PI/105 + 2.*PI**2/3 | ||
x5b = (-278185./33264 + 41*PI**2/96)*eta - 20261.*eta**2/2772 + 114635.*eta**3/99792 | ||
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x5log = - 428.*log(16*x)/105 | ||
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xarr5 = (x5a) + x5b | ||
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pre = sqrt(16.*PI/5) * 2 * eta | ||
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pn = xarr0 + x*xarr1 + x**(3/2.)*xarr2 + x**2*xarr3 + x**(5/2.)*xarr4 + x**3*(xarr5 + x5log) | ||
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return abs(pre * pn * x) | ||
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@vectorize(['float64(float64,float64,float64,float64,float64,float64,float64)'],target='cuda') | ||
def amp_ins_ansatz(t, eta, tc, a0, a1, b, c): | ||
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tau = (tc-t) | ||
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GW22AngFreq = freq_ins_ansatz(t, eta, tc, b, c, 1.) | ||
OrgAngFreq = GW22AngFreq / 2. | ||
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M = 1. | ||
x = (M*OrgAngFreq)**(2./3.) | ||
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T3amp = Hhat22_x(x, eta) | ||
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model = T3amp + a0*tau**(-9./8.) + a1*tau**(-10./8.) | ||
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return model |