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compton.c
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compton.c
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#include "decs.h"
/*
Routines for treating Compton scattering via Monte Carlo.
Sampling procedures for electron distribution is based on
Canfield, Howard, and Liang, 1987, ApJ 323, 565.
*/
/*
given photon w/ wavevector $k$ colliding w/ electron with
momentum $p$, ($p$ is actually the four-velocity)
find new wavevector $kp$
*/
#define OLD_E_SAMP (0)
void sample_scattered_photon(double k[4], double p[4], double kp[4])
{
double ke[4], kpe[4];
double k0p;
double n0x, n0y, n0z, n0dotv0, v0x, v0y, v0z, v1x, v1y, v1z, v2x,
v2y, v2z, v1, dir1, dir2, dir3;
double cth, sth, phi, cphi, sphi;
void sincos(double x, double *sin, double *cos);
/* boost into the electron frame
ke == photon momentum in elecron frame */
boost(k, p, ke);
if (ke[0] > 1.e-4) {
k0p = sample_klein_nishina(ke[0]);
cth = 1. - 1 / k0p + 1. / ke[0];
} else {
k0p = ke[0];
cth = sample_thomson();
}
sth = sqrt(fabs(1. - cth * cth));
/* unit vector 1 for scattering coordinate system is
oriented along initial photon wavevector */
//v0x = ke[1] / ke[0];
//v0y = ke[2] / ke[0];
//v0z = ke[3] / ke[0];
// Explicitly compute kemag instead of using ke[0] to ensure that photon
// is created normalized and doesn't inherit light cone errors from the
// original superphoton
double kemag = sqrt(ke[1]*ke[1] + ke[2]*ke[2] + ke[3]*ke[3]);
v0x = ke[1]/kemag;
v0y = ke[2]/kemag;
v0z = ke[3]/kemag;
/* randomly pick zero-angle for scattering coordinate system.
There's undoubtedly a better way to do this. */
monty_ran_dir_3d(&n0x, &n0y, &n0z);
n0dotv0 = v0x * n0x + v0y * n0y + v0z * n0z;
/* unit vector 2 */
v1x = n0x - (n0dotv0) * v0x;
v1y = n0y - (n0dotv0) * v0y;
v1z = n0z - (n0dotv0) * v0z;
v1 = sqrt(v1x * v1x + v1y * v1y + v1z * v1z);
v1x /= v1;
v1y /= v1;
v1z /= v1;
/* find one more unit vector using cross product;
this guy is automatically normalized */
v2x = v0y * v1z - v0z * v1y;
v2y = v0z * v1x - v0x * v1z;
v2z = v0x * v1y - v0y * v1x;
/* now resolve new momentum vector along unit vectors */
/* create a four-vector $p$ */
/* solve for orientation of scattered photon */
/* find phi for new photon */
phi = 2. * M_PI * monty_rand();
sincos(phi, &sphi, &cphi);
p[1] *= -1.;
p[2] *= -1.;
p[3] *= -1.;
dir1 = cth * v0x + sth * (cphi * v1x + sphi * v2x);
dir2 = cth * v0y + sth * (cphi * v1y + sphi * v2y);
dir3 = cth * v0z + sth * (cphi * v1z + sphi * v2z);
kpe[0] = k0p;
kpe[1] = k0p * dir1;
kpe[2] = k0p * dir2;
kpe[3] = k0p * dir3;
/* transform k back to lab frame */
boost(kpe, p, kp);
/* quality control */
if (kp[0] < 0 || isnan(kp[0])) {
fprintf(stderr, "in sample_scattered_photon:\n");
fprintf(stderr, "kp[0], kpe[0]: %g %g\n", kp[0], kpe[0]);
fprintf(stderr, "kpe: %g %g %g %g\n", kpe[0], kpe[1],
kpe[2], kpe[3]);
fprintf(stderr, "k: %g %g %g %g\n", k[0], k[1], k[2],
k[3]);
fprintf(stderr, "ke: %g %g %g %g\n", ke[0], ke[1], ke[2],
ke[3]);
fprintf(stderr, "p: %g %g %g %g\n", p[0], p[1], p[2],
p[3]);
fprintf(stderr, "kp: %g %g %g %g\n", kp[0], kp[1], kp[2],
kp[3]);
}
/* done! */
}
/*
Lorentz boost vector v into frame given by four-velocity u.
Result goes out in vp.
Assumes all four-velocities are given in orthonormal coordinates.
*/
void boost(double v[4], double u[4], double vp[4])
{
double g, V, n1, n2, n3, gm1;
g = u[0];
V = sqrt(fabs(1. - 1. / (g * g)));
n1 = u[1] / (g * V + SMALL);
n2 = u[2] / (g * V + SMALL);
n3 = u[3] / (g * V + SMALL);
gm1 = g - 1.;
/* general Lorentz boost into frame u from lab frame */
vp[0] = u[0]*v[0] -
u[1]*v[1] -
u[2]*v[2] -
u[3]*v[3];
vp[1] = -u[1] * v[0] +
(1. + n1 * n1 * gm1) * v[1] +
n1 * n2 * gm1 * v[2] +
n1 * n3 * gm1 * v[3];
vp[2] = -u[2] * v[0] +
n2 * n1 * gm1 * v[1] +
(1. + n2 * n2 * gm1) * v[2] +
n2 * n3 * gm1 * v[3];
vp[3] = -u[3] * v[0] +
n3 * n1 * gm1 * v[1] +
n3 * n2 * gm1 * v[2] +
(1. + n3 * n3 * gm1) * v[3];
}
/* return a cos(theta) consistent w/ Thomson
differential cross section */
/* uses simple rejection scheme */
double sample_thomson()
{
double x1, x2;
do {
x1 = 2. * monty_rand() - 1.;
x2 = (3. / 4.) * monty_rand();
} while (x2 >= (3. / 8.) * (1. + x1 * x1));
return (x1);
}
/*
sample Klein-Nishina differential cross section.
This routine is inefficient; it needs improvement.
*/
double sample_klein_nishina(double k0)
{
double k0pmin, k0pmax, k0p_tent, x1;
int n = 0;
/* a low efficiency sampling algorithm, particularly for large k0;
limiting efficiency is log(2 k0)/(2 k0) */
k0pmin = k0 / (1. + 2. * k0); /* at theta = Pi */
k0pmax = k0; /* at theta = 0 */
do {
/* tentative value */
k0p_tent = k0pmin + (k0pmax - k0pmin) * monty_rand();
/* rejection sample in box of height = kn(kmin) */
x1 = 2. * (1. + 2. * k0 +
2. * k0 * k0) / (k0 * k0 * (1. + 2. * k0));
x1 *= monty_rand();
n++;
} while (x1 >= klein_nishina(k0, k0p_tent));
return (k0p_tent);
}
/*
differential cross section for scattering from
frequency a -> frequency ap. Frequencies are
in units of m_e. Unnormalized!
*/
double klein_nishina(double a, double ap)
{
double ch, kn;
ch = 1. + 1. / a - 1. / ap;
kn = (a / ap + ap / a - 1. + ch * ch) / (a * a);
return (kn);
}
/*
sample electron distribution to find which electron was
scattered.
*/
void sample_electron_distr_p(double k[4], double p[4], double Thetae)
{
double beta_e, mu, phi, cphi, sphi, gamma_e, sigma_KN;
double K, sth, cth, x1, n0dotv0, v0, v1;
double n0x, n0y, n0z;
double v0x, v0y, v0z;
double v1x, v1y, v1z;
double v2x, v2y, v2z;
int sample_cnt = 0;
void sincos(double x, double *sin, double *cos);
do {
sample_beta_distr(Thetae, &gamma_e, &beta_e);
mu = sample_mu_distr(beta_e);
/* sometimes |mu| > 1 from roundoff error, fix it */
if (mu > 1.)
mu = 1.;
else if (mu < -1.)
mu = -1;
/* frequency in electron rest frame */
K = gamma_e * (1. - beta_e * mu) * k[0];
/* Avoid problems at small K */
if (K < 1.e-3) {
sigma_KN = 1. - 2. * K;
} else {
/* Klein-Nishina cross-section / Thomson */
sigma_KN = (3. / (4. * K * K)) * (2. +
K * K * (1. +
K) / ((1. +
2. *
K) *
(1. +
2. *
K)) +
(K * K - 2. * K -
2.) / (2. * K) *
log(1. + 2. * K));
}
x1 = monty_rand();
sample_cnt++;
if (sample_cnt > 10000000) {
fprintf(stderr,
"in sample_electron mu, gamma_e, K, sigma_KN, x1: %g %g %g %g %g %g\n",
Thetae, mu, gamma_e, K, sigma_KN, x1);
/* This is a kluge to prevent stalling for large values of \Theta_e */
Thetae *= 0.5;
sample_cnt = 0;
}
} while (x1 >= sigma_KN);
/* first unit vector for coordinate system */
v0x = k[1];
v0y = k[2];
v0z = k[3];
v0 = sqrt(v0x * v0x + v0y * v0y + v0z * v0z);
v0x /= v0;
v0y /= v0;
v0z /= v0;
/* pick zero-angle for coordinate system */
monty_ran_dir_3d(&n0x, &n0y, &n0z);
n0dotv0 = v0x * n0x + v0y * n0y + v0z * n0z;
/* second unit vector */
v1x = n0x - (n0dotv0) * v0x;
v1y = n0y - (n0dotv0) * v0y;
v1z = n0z - (n0dotv0) * v0z;
/* normalize */
v1 = sqrt(v1x * v1x + v1y * v1y + v1z * v1z);
v1x /= v1;
v1y /= v1;
v1z /= v1;
/* find one more unit vector using cross product;
this guy is automatically normalized */
v2x = v0y * v1z - v0z * v1y;
v2y = v0z * v1x - v0x * v1z;
v2z = v0x * v1y - v0y * v1x;
/* now resolve new momentum vector along unit vectors
and create a four-vector $p$ */
phi = monty_rand() * 2. * M_PI; /* orient uniformly */
sincos(phi, &sphi, &cphi);
cth = mu;
sth = sqrt(1. - mu * mu);
p[0] = gamma_e;
p[1] = gamma_e * beta_e * (cth * v0x +
sth * (cphi * v1x + sphi * v2x));
p[2] = gamma_e * beta_e * (cth * v0y +
sth * (cphi * v1y + sphi * v2y));
p[3] = gamma_e * beta_e * (cth * v0z +
sth * (cphi * v1z + sphi * v2z));
if (beta_e < 0) {
fprintf(stderr, "betae error: %g %g %g %g\n",
p[0], p[1], p[2], p[3]);
}
return;
}
/*
sample dimensionless speed of electron
from relativistic maxwellian
checked.
*/
struct df_params {
double Thetae;
};
// Function that, when zero, gives gamma for which dN/d log gam is maximized
double dfdgam(double ge, void *params)
{
struct df_params *p = (struct df_params*) params;
double Te = p->Thetae;
#if DIST_KAPPA
double kap = KAPPA;
//return ((2.-3*ge*ge)*kap*Te + (ge-1)*(ge*(ge*(kap-2.)+kap+1)+2.));
double gc = GAMMACUT;
return (1.-ge)*ge*(-ge+ge*ge*ge+gc*(2.+ge*(1.+ge*(-2.+kap)+kap))) + ge*(ge-ge*ge*ge+gc*(-2.+3.*ge*ge))*kap*Te;
#else
return ge - pow(ge,3.) - 2.*Te + 3.*pow(ge,2.)*Te;
#endif
}
// Maxwell-Juettner distribution, prefactor removed for sampling
// dN / d \log \gamma
double fdist(double ge, double Thetae)
{
#if DIST_KAPPA
double kap = KAPPA;
return pow(ge,2)*sqrt(ge*ge-1.)*pow(1. + (ge-1.)/(kap*Thetae),-kap-1.)*exp(-ge/GAMMACUT);
#else
return ge*ge*sqrt(ge*ge-1.)*exp(-ge/Thetae);
#endif
}
#include <gsl/gsl_errno.h>
#include <gsl/gsl_math.h>
#include <gsl/gsl_roots.h>
void sample_beta_distr(double Thetae, double *gamma_e, double *beta_e)
{
#if OLD_E_SAMP
// Sanity check
#if DIST_KAPPA
printf("Can't use old E sampling with kappa distribution!\n");
exit(-1);
#endif
double y;
/* checked */
y = sample_y_distr(Thetae);
/* checked */
*gamma_e = y * y * Thetae + 1.;
*beta_e = sqrt(1. - 1. / (*gamma_e * *gamma_e));
return;
#else
// Relativistic kappa distribution does not like very small Thetae. Ugly kludge.
if (Thetae < 0.01) {
*gamma_e = 1.000001;
*beta_e = sqrt(1. - 1. / (*gamma_e * *gamma_e));
return;
}
// Get maximum for window
int status, iter = 0, max_iter = 100;
const gsl_root_fsolver_type *T;
gsl_root_fsolver *s;
double ge_max = 1. + Thetae;
double ge_lo = GSL_MAX(1., 0.01*Thetae);
double ge_hi = GSL_MAX(100., 1000.*Thetae);
//printf("Thetae = %e ge_lo = %e ge_hi = %e\n", Thetae, ge_lo, ge_hi);
gsl_function F;
struct df_params params = {Thetae};
//printf("%e %e\n", dfdgam(ge_lo, ¶ms), dfdgam(ge_hi, ¶ms));
F.function = &dfdgam;
F.params = ¶ms;
T = gsl_root_fsolver_brent;
s = gsl_root_fsolver_alloc(T);
gsl_root_fsolver_set(s, &F, ge_lo, ge_hi);
do {
iter++;
status = gsl_root_fsolver_iterate(s);
ge_max = gsl_root_fsolver_root(s);
ge_lo = gsl_root_fsolver_x_lower(s);
ge_hi = gsl_root_fsolver_x_upper(s);
status = gsl_root_test_interval(ge_lo, ge_hi, 0, 0.001);
} while (status == GSL_CONTINUE && iter < max_iter);
//printf("ge_max = %e\n", ge_max);
double f_max = fdist(ge_max, Thetae);
//printf("fmax = %e\n", f_max);
gsl_root_fsolver_free(s);
// Sample electron gamma
double ge_samp;
do {
double lge_min = log(GSL_MAX(1., 0.01*Thetae));
double lge_max = log(GSL_MAX(100., 1000.*Thetae));
ge_samp = exp(lge_min + (lge_max - lge_min)*monty_rand());
} while (fdist(ge_samp, Thetae)/f_max < monty_rand());
//printf("ge_samp = %e\n", ge_samp);
*gamma_e = ge_samp;
*beta_e = sqrt(1. - 1. / (*gamma_e * *gamma_e));
//exit(-1);
#endif
}
/*
sample y, which is the temperature-normalized
kinetic energy.
Uses procedure outlined in Canfield et al. 1987,
p. 572 et seq.
*/
double sample_y_distr(double Thetae)
{
double S_3, pi_3, pi_4, pi_5, pi_6, y, x1, x2, x, prob;
double num, den;
pi_3 = sqrt(M_PI) / 4.;
pi_4 = sqrt(0.5 * Thetae) / 2.;
pi_5 = 3. * sqrt(M_PI) * Thetae / 8.;
pi_6 = Thetae * sqrt(0.5 * Thetae);
S_3 = pi_3 + pi_4 + pi_5 + pi_6;
pi_3 /= S_3;
pi_4 /= S_3;
pi_5 /= S_3;
pi_6 /= S_3;
do {
x1 = monty_rand();
if (x1 < pi_3) {
x = monty_ran_chisq(3);
} else if (x1 < pi_3 + pi_4) {
x = monty_ran_chisq(4);
} else if (x1 < pi_3 + pi_4 + pi_5) {
x = monty_ran_chisq(5);
} else {
x = monty_ran_chisq(6);
}
/* this translates between defn of distr in
Canfield et al. and standard chisq distr */
y = sqrt(x / 2);
x2 = monty_rand();
num = sqrt(1. + 0.5 * Thetae * y * y);
den = (1. + y * sqrt(0.5 * Thetae));
prob = num / den;
} while (x2 >= prob);
return (y);
}
double sample_mu_distr(double beta_e)
{
double mu, x1, det;
x1 = monty_rand();
det = 1. + 2. * beta_e + beta_e * beta_e - 4. * beta_e * x1;
if (det < 0.)
fprintf(stderr, "det < 0 %g %g\n\n", beta_e, x1);
mu = (1. - sqrt(det)) / beta_e;
return (mu);
}