def kepler_trig_expand(s):
"""
Transform trigonometric part of series s [sin(nM) and cos(nM)]
to sum of items like cos(M)^k1 * sin(M)^k2, where n=k1+k2.
- s is series of e and M,
- n is number of terms.
"""
from math import ceil
from pyranha.math import binomial, cos, sin, degree
temp, e, M, ecosM, esinM = 0, epst('e'), epst('M'), epst('ecosM'), epst(
'esinM')
n = degree(s).numerator
s_list = s.list
for i in range(len(s_list)):
for j in range(n + 1):
trig_cos, trig_sin = 0, 0
# calculate cos(nM):
if s_list[i][1] == cos(j * M):
for k in range(int(ceil(j / 2)) + 1):
trig_cos = trig_cos + (-1)**k * binomial(
j, 2 * k) * ecosM**(j - 2 * k) * esinM**(2 * k) * e**-j
temp = temp + s_list[i][0] * trig_cos
# calculate sin(nM):
if s_list[i][1] == sin(j * M):
for k in range(int(ceil((j - 1) / 2)) + 1):
trig_sin = trig_sin + (-1)**k * binomial(
j, 2 * k + 1) * ecosM**(j - 2 * k -
1) * esinM**(2 * k + 1) * e**-j
temp = temp + s_list[i][0] * trig_sin
if type(temp) != type(1): temp = temp.trim()
return temp
def a_r(e, M, order):
"""
Celestial mechanics classical expansion of a/r.
"""
from pyranha.math import cos
from fractions import Fraction as F
temp = 1
for k in range(1, order + 1):
temp = temp + F(2, 1) * besselJ(k, k * e, order) * cos(k * M)
return temp
def cos_E(e, M, order):
"""
Celestial mechanics classical expansion of cosE.
"""
from pyranha.math import cos
from fractions import Fraction as F
temp = F(-1, 2) * e
for k in range(1, order + 2):
temp = temp + F(1, k) * (besselJ(k - 1, k * e, order) -
besselJ(k + 1, k * e, order)) * cos(k * M)
return temp
def r_a(e, M, order):
"""
Celestial mechanics classical expansion of r/a.
"""
from pyranha.math import cos
from fractions import Fraction as F
temp = 1 + F(1, 2) * e**2
for k in range(1, order + 1):
temp = temp - e * F(1, k) * (besselJ(k - 1, k * e, order - 1) -
besselJ(k + 1, k * e, order - 1)) * cos(
k * M)
return temp
def cos_f(e, M, order):
"""
Celestial mechanics classical expansion of cosf.
"""
from pyranha.math import cos
temp = 0
for k in range(1, order + 2):
temp = temp + (besselJ(k - 1, k * e, order) +
besselJ(k + 1, k * e, order)) * cos(k * M)
temp = temp * (1 - e**2) - e
return temp.transform(
lambda t: (t[0].filter(lambda u: u[1].degree(['e']) <= order), t[1]))
def rrr(q, n, deg):
"""
Calculation expansions for r and them powers.
- n is maximum degree of variables.
"""
from pyranha.math import cos, sin
from eps.keproc import binomial_exp, r_a
deg_max, e_max = n / 2 + 1, n
MM, LL, xx, yy, uu, vv, qq = [
epst(i + str(q)) for i in ('m', 'L', 'x', 'y', 'u', 'v', 'q')
]
K0, ee, MA = epst('K0'), epst('e'), epst('M')
S1 = epst('s' + str(q - 1)) if q != 1 else F(1, 1)
S2 = epst('s' + str(q))
##################################################
temp2 = binomial_exp(epst(1), -epst('eps'), F(1, 2), deg_max)
temp5 = LL**F(-1, 2) * temp2.subs('eps',
F(1, 4) * LL**-1 * (xx**2 + yy**2))
ecospi = xx * temp5
esinpi = -yy * temp5
##################################################
ra = r_a(ee, MA, e_max)
ra = kepler_trig_expand(ra)
ra = ra.subs('e', ee**F(1, 2))
subs1 = ecospi * cos(qq) + esinpi * sin(qq)
subs2 = ecospi * sin(qq) - esinpi * cos(qq)
subs3 = LL**-1 * (xx**2 + yy**2) * (1 - F(1, 4) * LL**-1 * (xx**2 + yy**2))
##################################################
pt.set_auto_truncate_degree(F(n), ['x' + str(q), 'y' + str(q)])
ra = ra.subs('ecosM', subs1)
ra = ra.subs('esinM', subs2)
ra = ra.subs('e', subs3)
ra = ra.trim()
aa = (K0 * MM**2 * S1)**-1 * S2 * LL**2
ra_deg = (ra * aa)**deg
pt.unset_auto_truncate_degree()
return ra_deg.trim()
def one_r(p, n, deg):
"""
Calculation expansions for 1/r and their powers (deg).
- n is maximum degree of variables.
"""
from pyranha.math import cos, sin
from eps.keproc import binomial_exp, a_r
deg_max, e_max = n / 2 + 1, n
MM, LL, xx, yy, uu, vv, qq = [
epst(i + str(p)) for i in ('m', 'L', 'x', 'y', 'u', 'v', 'q')
]
K0, ee, MA = epst('K0'), epst('e'), epst('M')
S1 = epst('s' + str(p - 1)) if p != 1 else F(1, 1)
S2 = epst('s' + str(p))
########################################################################
temp2 = binomial_exp(epst(1), -epst('eps'), F(1, 2), deg_max)
temp5 = LL**F(-1, 2) * temp2.subs('eps',
F(1, 4) * LL**-1 * (xx**2 + yy**2))
ecospi = xx * temp5
esinpi = -yy * temp5
########################################################################
ar = a_r(ee, MA, e_max)
ar = kepler_trig_expand(ar)
ar = ar.subs('e', ee**F(1, 2))
subs1 = ecospi * cos(qq) + esinpi * sin(qq)
subs2 = ecospi * sin(qq) - esinpi * cos(qq)
subs3 = LL**-1 * (xx**2 + yy**2) * (1 - F(1, 4) * LL**-1 * (xx**2 + yy**2))
########################################################################
pt.set_auto_truncate_degree(F(n), ['x' + str(p), 'y' + str(p)])
ar = ar.subs('ecosM', subs1)
ar = ar.subs('esinM', subs2)
ar = ar.subs('e', subs3)
ar = ar.trim()
aa = (K0 * MM**2 * S1)**-1 * S2 * LL**2
ar_deg = (ar * aa**-1)**deg
pt.unset_auto_truncate_degree()
return ar_deg.trim()
def xyz(p, n):
"""
Calculation expansions for vector of x, y, z-coordinates.
- n is maximum degree of variables.
"""
from pyranha.math import cos, sin
from eps.keproc import binomial_exp, cos_E, sin_E
deg_max, e_max = n / 2 + 1, n
MM, LL, xx, yy, uu, vv, qq = [
epst(i + str(p)) for i in ('m', 'L', 'x', 'y', 'u', 'v', 'q')
]
K0, ee, MA, ecosM, esinM = epst('K0'), epst('e'), epst('M'), epst(
'ecosM'), epst('esinM')
S1 = epst('s' + str(p - 1)) if p != 1 else F(1, 1)
S2 = epst('s' + str(p))
##################################################
temp1 = binomial_exp(epst(1), -epst('eps'), -1, deg_max)
temp2 = binomial_exp(epst(1), -epst('eps'), F(1, 2), deg_max)
temp3 = F(1, 4) * LL**-1 * temp1.subs('eps',
F(1, 2) * LL**-1 * (xx**2 + yy**2))
temp5 = LL**F(-1, 2) * temp2.subs('eps',
F(1, 4) * LL**-1 * (xx**2 + yy**2))
temp4 = LL**F(-1,2) * temp1.subs('eps', F(1,2)*LL**-1 * (xx**2 + yy**2)) * \
temp2.subs('eps', F(1,4)*LL**-1 * (2*(xx**2 + yy**2) + (uu**2 + vv**2)))
cos2I = 1 - (uu**2 + vv**2) * temp3
sin2Icos2Om = (uu**2 - vv**2) * temp3
sin2Isin2Om = -2 * (uu * vv) * temp3
sinIsinOm = -vv * temp4
sinIcosOm = uu * temp4
ecospi = xx * temp5
esinpi = -yy * temp5
##################################################
temp = binomial_exp(epst(1), -ee**2, F(1, 2), e_max)
sqrt1 = F(1, 2) * (1 + temp)
sqrt2 = F(1, 2) * (1 - temp)
cosEM1 = cos_E(ee, MA, e_max) * cos(MA) + sin_E(ee, MA, e_max) * sin(MA)
cosEM2 = cos_E(ee, MA, e_max) * cos(MA) - sin_E(ee, MA, e_max) * sin(MA)
sinEM1 = sin_E(ee, MA, e_max) * cos(MA) - cos_E(ee, MA, e_max) * sin(MA)
sinEM2 = sin_E(ee, MA, e_max) * cos(MA) + cos_E(ee, MA, e_max) * sin(MA)
cosEM1 = (sqrt1 * cosEM1).truncate_degree(e_max, ['e'])
cosEM2 = (sqrt2 * cosEM2).truncate_degree(e_max, ['e'])
sinEM1 = (sqrt1 * sinEM1).truncate_degree(e_max, ['e'])
sinEM2 = (sqrt2 * sinEM2).truncate_degree(e_max, ['e'])
cosEM1 = kepler_trig_expand(cosEM1)
cosEM2 = kepler_trig_expand(cosEM2)
sinEM1 = kepler_trig_expand(sinEM1)
sinEM2 = kepler_trig_expand(sinEM2)
X_a = -ecosM + cosEM1 + cosEM2
Y_a = esinM + sinEM1 - sinEM2
X_a = X_a.subs('e', ee**F(1, 2))
Y_a = Y_a.subs('e', ee**F(1, 2))
subs1 = ecospi * cos(qq) + esinpi * sin(qq)
subs2 = ecospi * sin(qq) - esinpi * cos(qq)
subs3 = LL**-1 * (xx**2 + yy**2) * (1 - F(1, 4) * LL**-1 * (xx**2 + yy**2))
##################################################
pt.set_auto_truncate_degree(
F(n), ['x' + str(p), 'y' + str(p), 'u' + str(p), 'v' + str(p)])
X_a = X_a.subs('ecosM', subs1)
X_a = X_a.subs('esinM', subs2)
X_a = X_a.subs('e', subs3)
Y_a = Y_a.subs('ecosM', subs1)
Y_a = Y_a.subs('esinM', subs2)
Y_a = Y_a.subs('e', subs3)
aa = (K0 * MM**2 * S1)**-1 * S2 * LL**2
xa = aa * (X_a * (cos2I * cos(qq) + sin2Icos2Om * cos(qq) + sin2Isin2Om * sin(qq)) -\
Y_a * (cos2I * sin(qq) + sin2Icos2Om * sin(qq) - sin2Isin2Om * cos(qq)))
ya = aa * (X_a * (cos2I * sin(qq) - sin2Icos2Om * sin(qq) + sin2Isin2Om * cos(qq)) +\
Y_a * (cos2I * cos(qq) - sin2Icos2Om * cos(qq) - sin2Isin2Om * sin(qq)))
za = aa * (X_a * (sinIcosOm * sin(qq) - sinIsinOm * cos(qq)) +\
Y_a * (sinIcosOm * cos(qq) + sinIsinOm * sin(qq)))
pt.unset_auto_truncate_degree()
return [xa.trim(), ya.trim(), za.trim()]
def __init__(self,params = __default_params):
from numpy import dot
from mpmath import mpf
from fractions import Fraction as Frac
import sympy
from IPython.parallel import Client
# Set up constants.
self.__eps_val = (1./mpf(299792458.))**2
self.__GG_val = mpf(6.673E-11)
# Various variables.
Gt,I1,GG,m2,L,r,a,v2,Gtxy,ht,Ht,Gxy,h,H,J2,g,G,f,e,E,eps,hs,Hts,Gtxys = [pt(name) for name in ['\\tilde{G}','\\mathcal{I}_1',\
'\\mathcal{G}','m_2','L','r','a','v2','\\tilde{G}_{xy}','\\tilde{h}','\\tilde{H}','G_{xy}','h','H','J_2','g','G','f','e','E',\
'\\varepsilon','h_\\ast','\\tilde{H}_\\ast','\\tilde{G}_{xy\\ast}']]
# The unperturbed Hamiltonian.
H0 = Gt**2 * I1 / 2 - GG**2 * m2**2 * L**-2 / 2
self.__HH0 = H0
# Pieces of the perturbed Hamiltonian.
Gt_vec = [Gtxy * math.sin(ht),-Gtxy * math.cos(ht),Ht]
J2_vec = [0,0,J2]
r_vec = dot(celmec.orbitalR([math.cos(g),math.sin(g),H*G**-1,Gxy*G**-1,math.cos(h),math.sin(h)]),[r*math.cos(f),r*math.sin(f),0])
r_cross_v = [Gxy * math.sin(h),-Gxy * math.cos(h),H]
H1 = -Frac(1,8) * v2 ** 2 - Frac(3,2) * v2 * GG * m2 * r ** -1 + Frac(1,2) * GG**2 * m2**2 * r**-2 +\
Frac(3,2) * GG * m2 * r**-3 * dot(Gt_vec,r_cross_v) + 2 * GG * r**-3 * dot(J2_vec,r_cross_v) +\
GG * r**-3 * (3 * dot(Gt_vec,r_vec) * dot(J2_vec,r_vec) * r**-2 - dot(Gt_vec,J2_vec))
H1 = H1.subs('v2',GG * m2 * (2 * r**-1 - a ** -1)).subs('a',L ** 2 * (GG * m2)**-1)
# Verify formula in the paper.
assert(-Frac(1,8)*GG**4*m2**4*L**-4+r**-1*2*GG**3*m2**3*L**-2-r**-2*3*GG**2*m2**2+GG*r**-3*(\
2*J2*H+3*J2*Gxy**2*Ht*(G**-2)/2+3*m2*Ht*H/2-J2*Ht+(3*m2/2*Gtxy*Gxy-3*J2/2*H*Gxy*Gtxy*G**-2)*math.cos(ht-h)+\
3*J2*(-Frac(1,2)*Gxy**2*Ht*G**-2*math.cos(2*f+2*g)-Frac(1,4)*Gxy*Gtxy*G**-1*(1-H*G**-1)*math.cos(2*f+2*g+ht-h)+\
Frac(1,4)*Gxy*Gtxy*G**-1*(1+H*G**-1)*math.cos(2*f+2*g-ht+h))) == H1)
# Split the Hamiltonian in parts.
A0 = H1.transform(lambda t: (t[0].filter(lambda t: t[1].degree(['r']) == 0),t[1])).filter(lambda t: t[1] == pt(1)).subs('r',pt(1))
A1 = H1.transform(lambda t: (t[0].filter(lambda t: t[1].degree(['r']) == -1),t[1])).filter(lambda t: t[1] == pt(1)).subs('r',pt(1))
A2 = H1.transform(lambda t: (t[0].filter(lambda t: t[1].degree(['r']) == -2),t[1])).filter(lambda t: t[1] == pt(1)).subs('r',pt(1))
A3a = H1.transform(lambda t: (t[0].filter(lambda t: t[1].degree(['r']) == -3),t[1])).filter(lambda t: t[1] == pt(1)).subs('r',pt(1))
A3b = H1.filter(lambda t: t[1] == math.cos(ht - h)).transform(lambda t: (t[0],pt(1))).subs('r',pt(1))
B0 = H1.filter(lambda t: t[1] == math.cos(2*f + 2*g)).transform(lambda t: (t[0],pt(1))).subs('r',pt(1))
B1 = H1.filter(lambda t: t[1] == math.cos(2*f + 2*g + ht - h)).transform(lambda t: (t[0],pt(1))).subs('r',pt(1))
B2 = H1.filter(lambda t: t[1] == math.cos(2*f + 2*g - ht + h)).transform(lambda t: (t[0],pt(1))).subs('r',pt(1))
# Make sure we got them right.
assert(A0 + A1 * r**-1 + A2 * r**-2 + r**-3 * (A3a + A3b * math.cos(ht - h)) + r**-3 * (B0 * math.cos(2*f + 2*g) +\
B1 * math.cos(2*f + 2*g + ht - h) + B2 * math.cos(2*f + 2*g - ht + h)) == H1)
# This is the integrand in f (without the part that is integrated in E).
f_int = A2 * r**-2 + r**-3 * (A3a + A3b * math.cos(ht - h)) + r**-3 * (B0 * math.cos(2*f + 2*g) + B1 * math.cos(2*f + 2*g + ht - h) + B2 * math.cos(2*f + 2*g - ht + h))
# Change the integration variable to f (with the constant parts already taken out of the integral).
f_int *= r**2
# Substitute the definition of 1/r in terms of f.
f_int = f_int.subs('r',pt('rm1')**-1).subs('rm1',GG*m2*G**-2*(1+e*math.cos(f)))
# This is the integrand in E.
E_int = A1 * r**-1
# Change the integration variable to f.
E_int *= r**2
# Change the integration variable to E.
E_int *= L*G*r**-1*GG**-1*m2**-1
assert(E_int == A1*G*L*GG**-1*m2**-1)
# K1.
K1 = GG**2 * m2**2 * G**-1 * L**-3 * (f_int + E_int).filter(lambda t: t[1].t_degree(['f']) == 0)
# K.
K = K1 + A0
# The generator.
chi = G**-1 * (E_int.integrate('E') + f_int.integrate('f')) - L**3 * GG**-2 * m2**-2 * K1.integrate('l')
# Verifiy that chi satisfies the homological equation, yielding K.
assert((math.pbracket(H0,chi,['L','G','H','\\tilde{G}','\\tilde{H}'],['l','g','h','\\tilde{g}','\\tilde{h}']) + H1)\
.subs('r',pt('rm1')**-1).subs('rm1',GG*m2*G**-2*(1+e*math.cos(f))) == K)
# This is the complete Hamiltonian, with the two coordinates compressed into a single one.
HHp = H0 + eps * K.subs('h',ht+hs).subs('\\tilde{H}',Hts-H).subs('\\tilde{G}_{xy}',Gtxys)
# Record it as a member.
self.__HHp = HHp
# F0 and F1.
F0 = HHp.filter(lambda t: t[1].t_degree(['h_\\ast']) == 0).transform(lambda t: (t[0].filter(lambda t: t[1].degree(['\\varepsilon']) == 1),t[1])).subs('\\varepsilon',pt(1))
F1 = HHp.filter(lambda t: t[1].t_degree(['h_\\ast']) == 1).transform(lambda t: (t[0].filter(lambda t: t[1].degree(['\\varepsilon']) == 1),t[1])).subs('\\varepsilon',pt(1)).subs('h_\\ast',pt(0))
assert(H0 + eps * F0 + eps * F1 * math.cos(pt('h_\\ast')) == H0 + eps * K.subs('h',ht+hs).subs('\\tilde{H}',Hts-H).subs('\\tilde{G}_{xy}',Gtxys))
self.__F0 = F0
self.__F1 = F1
# Quartic polynomial.
f4H = (eps**2 * F1 ** 2 - (pt('\\mathcal{H}^\\prime') - H0 - eps * F0)**2)\
.ipow_subs('G_{xy}',2,G**2-H**2)\
.ipow_subs('\\tilde{G}_{xy\\ast}',2,Gt**2-(Hts-H)**2)
a4 = f4H.transform(lambda t: (t[0].filter(lambda t: t[1].degree(['H']) == 0),t[1]))
a3 = f4H.transform(lambda t: (t[0].filter(lambda t: t[1].degree(['H']) == 1),t[1])).subs('H',pt(1)) / 4
a2 = f4H.transform(lambda t: (t[0].filter(lambda t: t[1].degree(['H']) == 2),t[1])).subs('H',pt(1)) / 6
a1 = f4H.transform(lambda t: (t[0].filter(lambda t: t[1].degree(['H']) == 3),t[1])).subs('H',pt(1)) / 4
a0 = f4H.transform(lambda t: (t[0].filter(lambda t: t[1].degree(['H']) == 4),t[1])).subs('H',pt(1))
# NOTE: these are not the polynomial coefficient strictly speaking, they are normalised by 4, 6 and 4
# as shown above and in the assert below.
self.__f4_cf = (a0,a1,a2,a3,a4)
# Check we got them right.
assert(a4+4*a3*H+6*a2*H**2+4*a1*H**3+a0*H**4 == f4H)
# Store the coefficients - from high degree to low.
self.__f4_coeffs = [t[0] * t[1].trim() for t in zip([1,4,6,4,1],self.__f4_cf)]
# Derivatives of the quartic poly.
f4Hp = math.partial(f4H,'H')
f4Hpp = math.partial(f4Hp,'H')
f4Hppp = math.partial(f4Hpp,'H')
f4Hpppp = math.partial(f4Hppp,'H')
# Check the derivatives for consistency.
assert(f4Hp == 4*a3 + 12*a2*H + 12*a1*H**2 + 4*a0*H**3)
assert(f4Hpp == 12*a2 + 24*a1*H + 12*a0*H**2)
assert(f4Hppp == 24*a1 + 24*a0*H)
assert(f4Hpppp == 24*a0)
self.__f4 = [f4H, f4Hp, f4Hpp, f4Hppp, f4Hpppp]
# Invariants for wp.
g2 = a0*a4 - 4*a1*a3 + 3*a2**2
g3 = a0*a2*a4 + 2*a1*a2*a3 - (a2**3) - (a0*a3**2) - (a1**2*a4)
self.__g2 = g2
self.__g3 = g3
# Solve the angles.
# Extract cosine of h_s.
#chs = sympy.solve((spin_gr_theory.__to_sympy(self.HHp.trim())-sympy.Symbol('\\mathcal{H}^\\prime')).replace(sympy.cos(sympy.Symbol('h_\\ast')),sympy.Symbol('chs')),sympy.Symbol('chs'))[0]
#ipy_view = Client().load_balanced_view()
#g_sol = ipy_view.apply_async(spin_gr_theory.__solve_g,chs,spin_gr_theory.__to_sympy(math.partial(self.HHp.trim(),'G')))
#hs_sol = ipy_view.apply_async(spin_gr_theory.__solve_hs,chs,spin_gr_theory.__to_sympy(math.partial(self.HHp.trim(),'H')))
#ht_sol = ipy_view.apply_async(spin_gr_theory.__solve_ht,chs,spin_gr_theory.__to_sympy(math.partial(self.HHp.trim(),'\\tilde{H}_\\ast')))
#self.__g_sol = g_sol.get()
#self.__hs_sol = hs_sol.get()
#self.__ht_sol = ht_sol.get()
import pickle
self.__g_sol = pickle.load(open('g_sol.pickle','rb'))
self.__hs_sol = pickle.load(open('hs_sol.pickle','rb'))
self.__ht_sol = pickle.load(open('ht_sol.pickle','rb'))
# Set the parameters of the theory.
self.__set_params(params)
# Some sanity checks.
HHp,G,L,H,GG,eps,m2,Hts,Gt,J2,hs,Gxy,Gtxys = [sympy.Symbol(s) for s in ['\\mathcal{H}^\\prime','G','L','H','\\mathcal{G}',\
'\\varepsilon','m_2','\\tilde{H}_\\ast','\\tilde{G}','J_2','h_\\ast','G_{xy}','\\tilde{G}_{xy\\ast}']]
# Phi_g^4 going to zero in the equilibrium point.
assert(self.g_sol[0][3][1].subs(HHp,spin_gr_theory.__to_sympy(self.HHp.ipow_subs('G_{xy}',2,pt('G')**2\
-pt('H')**2).subs('H',pt('G')**2*pt('m_2')*pt('J_2')**-1))).ratsimp() == 0)
# Reduction to Einstein precession.
simpl_HHp_ein = spin_gr_theory.__to_sympy(self.HHp.subs('J_2',0).subs('\\tilde{G}_{xy\\ast}',0).subs('\\tilde{H}_\\ast',pt('H'))\
.subs('\\tilde{G}',0))
ein_prec = sum([t[0]*t[1] for t in self.g_sol[0]]).subs('J_2',0).subs(Hts,H).subs(Gt,0)\
.subs(HHp,simpl_HHp_ein).ratsimp()
assert(ein_prec == 3 * eps * GG**4 * m2**4/(G**2*L**3))
# Lense-Thirring precession for g.
simpl_HHp_lt = spin_gr_theory.__to_sympy(self.HHp.subs('\\tilde{G}_{xy\\ast}',0).subs('\\tilde{H}_\\ast',pt('H'))\
.subs('\\tilde{G}',0))
lt_prec = sum([t[0]*t[1] for t in self.g_sol[0]]).subs(Hts,H).subs(Gt,0).subs(HHp,simpl_HHp_lt).ratsimp()
assert(lt_prec == (eps * ((-6*H*J2*GG**4*m2**3)/(G**4*L**3)+3*GG**4*m2**4/(G**2*L**3))).ratsimp())
# Geodetic effect on g.
simpl_HHp_ge = spin_gr_theory.__to_sympy(self.HHp.subs('J_2',0)).subs(sympy.cos(hs),-1).subs(Gxy,sympy.sqrt(G**2-H**2))\
.subs(Gtxys,sympy.sqrt(Gt**2-(Hts-H)**2)).subs(H,(Hts**2+G**2-Gt**2)/(2*Hts))
ge_g = sum([t[0]*t[1] for t in self.g_sol[0]]).subs(J2,0).subs(Gxy,sympy.sqrt(G**2-H**2))\
.subs(Gtxys,sympy.sqrt(Gt**2-(Hts-H)**2)).subs(H,(Hts**2+G**2-Gt**2)/(2*Hts)).subs(HHp,simpl_HHp_ge).ratsimp()
assert(ge_g == (1 / (4*G**4*L**3) * (15*G**2*GG**4*eps*m2**4+9*GG**4*Gt**2*eps*m2**4-9*GG**4*Hts**2*eps*m2**4)).ratsimp())
# No precession in h for Einstein case.
assert((sum([t[0]*t[1] for t in self.hs_sol[0]]) + sum([t[0]*t[1] for t in self.ht_sol[0]])).subs(HHp,simpl_HHp_ein)\
.subs('J_2',0).subs(Hts,H).ratsimp().subs(Gt,0) == 0)
# h precession in LT.
assert((sum([t[0]*t[1] for t in self.hs_sol[0]]) + sum([t[0]*t[1] for t in self.ht_sol[0]])).subs(HHp,simpl_HHp_lt)\
.subs(Hts,H).ratsimp().subs(Gt,0).ratsimp() == 2*eps*J2*GG**4*m2**3/(G**3*L**3))
# Geodetic effect for h and ht.
assert((sum([t[0]*t[1] for t in self.hs_sol[0]]) + sum([t[0]*t[1] for t in self.ht_sol[0]])).subs(HHp,simpl_HHp_ge)\
.subs(J2,0).subs(H,(Hts**2+G**2-Gt**2)/(2*Hts)).ratsimp() == 3*GG**4*Hts*eps*m2**4/(2*G**3*L**3))
assert((sum([t[0]*t[1] for t in self.ht_sol[0]])).subs(HHp,simpl_HHp_ge)\
.subs(J2,0).subs(H,(Hts**2+G**2-Gt**2)/(2*Hts)).ratsimp() == 3*GG**4*Hts*eps*m2**4/(2*G**3*L**3))
