This test checks that active neutrinos do not get any non-equilibrium corrections at temperatures
import os
import numpy
import matplotlib
from plotting import plt
from particles import Particle
from library.SM import particles as SMP, interactions as SMI
from evolution import Universe
from common import UNITS, Params, GRID
folder = os.path.split(__file__)[0]
T_initial = 1000. * UNITS.MeV
T_final = 100 * UNITS.MeV
params = Params(T=T_initial,
dy=0.025)
universe = Universe(params=params, logfile=os.path.join(folder, 'log.txt'))
photon = Particle(**SMP.photon)
electron = Particle(**SMP.leptons.electron)
muon = Particle(**SMP.leptons.muon)
tau = Particle(**SMP.leptons.tau)
neutrino_e = Particle(**SMP.leptons.neutrino_e)
neutrino_mu = Particle(**SMP.leptons.neutrino_mu)
neutrino_tau = Particle(**SMP.leptons.neutrino_tau)
universe.add_particles([
photon,
electron,
muon,
tau,
neutrino_e,
neutrino_mu,
neutrino_tau,
])
neutrinos = [neutrino_e, neutrino_mu, neutrino_tau]
for neutrino in neutrinos:
neutrino.decoupling_temperature = T_initial
universe.interactions += \
SMI.neutrino_interactions(leptons=[electron, muon, tau], neutrinos=neutrinos)
universe.graphics.monitor(particles=neutrinos, plasma_distribution=True)
universe.evolve(T_final)
universe.graphics.save(__file__)
plt.figure(9)
plt.title('Figure 9')
plt.xlabel('MeV/T')
plt.ylabel(u'aT')
plt.xscale('log')
plt.xlim(0.5, UNITS.MeV/universe.params.T)
plt.xticks([1, 2, 3, 5, 10, 20])
plt.axes().get_xaxis().set_major_formatter(matplotlib.ticker.ScalarFormatter())
plt.plot(UNITS.MeV / numpy.array(universe.data['T']), numpy.array(universe.data['aT']) / UNITS.MeV)
plt.show()
plt.savefig(os.path.join(folder, 'figure_9.svg'))
plt.figure(10)
plt.title('Figure 10')
plt.xlabel('Conformal momentum y = pa')
plt.ylabel('f/f_eq')
plt.xlim(0, 20)
f_e = neutrino_e._distribution
feq_e = neutrino_e.equilibrium_distribution()
plt.plot(GRID.TEMPLATE/UNITS.MeV, f_e/feq_e, label="nu_e")
f_mu = neutrino_mu._distribution
feq_mu = neutrino_mu.equilibrium_distribution()
plt.plot(GRID.TEMPLATE/UNITS.MeV, f_mu/feq_mu, label="nu_mu")
f_tau = neutrino_tau._distribution
feq_tau = neutrino_tau.equilibrium_distribution()
plt.plot(GRID.TEMPLATE/UNITS.MeV, f_tau/feq_tau, label="nu_tau")
plt.legend()
plt.draw()
plt.show()
plt.savefig(os.path.join(folder, 'figure_10_full.svg'))
plt.xlim(0, 10)
plt.ylim(0.99, 1.06)
plt.draw()
plt.show()
plt.savefig(os.path.join(folder, 'figure_10.svg'))
Distribution functions arrays
distributions_file = open(os.path.join(folder, 'distributions.txt'), "w")
numpy.savetxt(distributions_file, (f_e, feq_e, f_e/feq_e), header=str(neutrino_e),
footer='-'*80, fmt="%1.5e")
numpy.savetxt(distributions_file, (f_mu, feq_mu, f_mu/feq_mu), header=str(neutrino_mu),
footer='-'*80, fmt="%1.5e")
numpy.savetxt(distributions_file, (f_tau, feq_tau, f_tau/feq_tau), header=str(neutrino_tau),
footer='-'*80, fmt="%1.5e")
distributions_file.close()