示例#1
0
def find_gamma(energy, jnu, Z=1):
    """ Find the photoionization rate / 1e12 given the spectrum as a
    function of energy in Rydbergs.

    in units of photons / s.

    This is copying JFH's code in cldy_cuba_jfh.pro.
    """

    sigma_nu = photo_cross_section_hydrogenic(energy, Z=Z)
    # output is in units of 1e-12
    integrand = 4. * pi * jnu * sigma_nu / hplanck * 1e12

    log_energy = np.log10(energy)
    isort = np.argsort(log_energy)
    # don't understand why this works...
    gamma = np.log(10) * simps(integrand[isort], x=log_energy[isort])
    return gamma
示例#2
0
def find_gamma(energy, jnu, Z=1):
    """ Find the photoionization rate / 1e12 given the spectrum as a
    function of energy in Rydbergs.

    in units of photons / s.

    This is copying JFH's code in cldy_cuba_jfh.pro.
    """

    sigma_nu = photo_cross_section_hydrogenic(energy, Z=Z)
    # output is in units of 1e-12
    integrand = 4. * pi * jnu * sigma_nu / hplanck * 1e12

    log_energy = np.log10(energy)
    isort = np.argsort(log_energy)
    # don't understand why this works...
    gamma = np.log(10) * simps(integrand[isort], x=log_energy[isort])
    return gamma
示例#3
0
    sigma_nu = photo_cross_section_hydrogenic(energy, Z=Z)
    # output is in units of 1e-12
    integrand = 4. * pi * jnu * sigma_nu / hplanck * 1e12

    log_energy = np.log10(energy)
    isort = np.argsort(log_energy)
    # don't understand why this works...
    gamma = np.log(10) * simps(integrand[isort], x=log_energy[isort])
    return gamma

if 0:
    # They match, woot!
    iHeII = 2
    E = 10**np.linspace(1, 5, 100) * u.eV
    s, Eth, Emax = sigma_Verner96(E, iHeII)
    s2 = photo_cross_section_hydrogenic(E.to(u.rydberg).value, Z=2)
    plt.loglog(E.value, s.value*1e18)
    plt.loglog(E.value, s2*1e18)
    show()

if 1:
    # measure the photoionization rate, which is the integral of the
    # ionizing field * the cross section.

    # from McQuinn and Worseck 2014MNRAS.440.2406M

    # eta = 0.43 * gamma_HI / gamma_HeII

    # Faucher-Giguere 2009
    gamma_HI = 0.861e-12
    print 'gamma HeII'
示例#4
0
    # output is in units of 1e-12
    integrand = 4. * pi * jnu * sigma_nu / hplanck * 1e12

    log_energy = np.log10(energy)
    isort = np.argsort(log_energy)
    # don't understand why this works...
    gamma = np.log(10) * simps(integrand[isort], x=log_energy[isort])
    return gamma


if 0:
    # They match, woot!
    iHeII = 2
    E = 10**np.linspace(1, 5, 100) * u.eV
    s, Eth, Emax = sigma_Verner96(E, iHeII)
    s2 = photo_cross_section_hydrogenic(E.to(u.rydberg).value, Z=2)
    plt.loglog(E.value, s.value * 1e18)
    plt.loglog(E.value, s2 * 1e18)
    show()

if 1:
    # measure the photoionization rate, which is the integral of the
    # ionizing field * the cross section.

    # from McQuinn and Worseck 2014MNRAS.440.2406M

    # eta = 0.43 * gamma_HI / gamma_HeII

    # Faucher-Giguere 2009
    gamma_HI = 0.861e-12
    print 'gamma HeII'