Пример #1
0
class TestCosmology(object):
    def setup(self):

        self.arcsec = 2 * np.pi / 360 / 3600
        self.zlens = 1
        self.zsource = 2
        self.angle_diameter = 2 / self.arcsec
        self.angle_radius = 0.5 * self.angle_diameter

        self.H0 = 70
        self.omega_baryon = 0.03
        self.omega_DM = 0.25
        self.sigma8 = 0.82
        curvature = 'flat'
        self.ns = 0.9608
        cosmo_params = {
            'H0': self.H0,
            'Om0': self.omega_baryon + self.omega_DM,
            'Ob0': self.omega_baryon,
            'sigma8': self.sigma8,
            'ns': self.ns,
            'curvature': curvature
        }
        self._dm, self._bar = self.omega_DM, self.omega_baryon
        self.cosmo = Cosmology(cosmo_kwargs=cosmo_params)
        self.geometry = Geometry(self.cosmo, self.zlens, self.zsource,
                                 self.angle_diameter, 'DOUBLE_CONE')

    def test_cosmo(self):

        da_true = self.cosmo.D_A(0, 1.824)
        da_interp = self.cosmo.D_A_z(1.824)
        npt.assert_almost_equal(da_true / da_interp, 1, 5)

        dc_true = self.cosmo.astropy.comoving_transverse_distance(1.4).value
        dc_interp = self.cosmo.D_C_z(1.4)
        dc_astropy = self.cosmo.astropy.comoving_distance(1.4).value
        npt.assert_almost_equal(dc_true / dc_interp, 1)
        npt.assert_almost_equal(dc_astropy / dc_true, 1)

        dc_transverse = self.cosmo.D_C_transverse(0.8)
        dc = self.cosmo.astropy.comoving_transverse_distance(0.8).value
        npt.assert_almost_equal(dc / dc_transverse, 1)

        ez = self.cosmo.E_z(0.8)
        ez_astropy = self.cosmo.astropy.efunc(0.8)
        npt.assert_almost_equal(ez / ez_astropy, 1)

        kpc_per_asec = self.cosmo.kpc_proper_per_asec(0.5)
        kpc_per_arcsec_true = self.cosmo.astropy.kpc_proper_per_arcmin(
            0.5).value / 60
        npt.assert_almost_equal(kpc_per_asec, kpc_per_arcsec_true, 2)

        rho_crit_0 = self.cosmo.rho_crit(0)
        rho_pc = un.Quantity(self.cosmo.astropy.critical_density(0),
                             unit=un.Msun / un.pc**3)
        rho_Mpc = rho_pc.value * (1e+6)**3
        npt.assert_almost_equal(rho_crit_0 / rho_Mpc, 1, 3)

        rho_crit = self.cosmo.rho_crit(0.6)
        rho_pc = un.Quantity(self.cosmo.astropy.critical_density(0.6),
                             unit=un.Msun / un.m**3)
        rho_Mpc = rho_pc.value * self.cosmo.Mpc**3
        npt.assert_almost_equal(rho_crit / rho_Mpc, 1, 3)

        rho_crit_dark_matter = self.cosmo.rho_dark_matter_crit
        rho_crit_DM_astropy = self.cosmo.astropy.critical_density(0.).value * \
                              self.cosmo.density_to_MsunperMpc * self.cosmo.astropy.Odm(0.)
        npt.assert_almost_equal(rho_crit_DM_astropy, rho_crit_dark_matter)

        rho_crit = self.cosmo.rho_crit(0.3)
        rho_pc = un.Quantity(self.cosmo.astropy.critical_density(0.3),
                             unit=un.Msun / un.pc**3)
        rho_Mpc = rho_pc.value * (1e+6)**3
        npt.assert_almost_equal(rho_crit / rho_Mpc, 1, 3)

        colossus = self.cosmo.colossus

        npt.assert_almost_equal(colossus.Om0,
                                self.omega_DM + self.omega_baryon)
        npt.assert_almost_equal(colossus.Ob0, self.omega_baryon)
        npt.assert_almost_equal(colossus.H0, self.H0)
        npt.assert_almost_equal(colossus.sigma8, self.sigma8)
        npt.assert_almost_equal(colossus.ns, self.ns)

        halo_collapse_z = 9.
        age_today = self.cosmo.astropy.age(0.).value
        age_z = self.cosmo.astropy.age(halo_collapse_z).value
        age = age_today - age_z
        npt.assert_almost_equal(age,
                                self.cosmo.halo_age(0., zform=halo_collapse_z))

        npt.assert_almost_equal(self.cosmo.scale_factor(0.7),
                                self.cosmo.astropy.scale_factor(0.7))
Пример #2
0
class TestLensCosmo(object):

    def setup(self):

        kwargs_cosmo = {'Om0': 0.2}
        self.cosmo = Cosmology(cosmo_kwargs=kwargs_cosmo)
        zlens, zsource = 0.3, 1.7
        self.lens_cosmo = LensCosmo(zlens, zsource, self.cosmo)
        self.h = self.cosmo.h
        self.con = Concentration(self.lens_cosmo)

        self._colossus_nfw = NFWProfile

    def test_const(self):

        D_ds = self.cosmo.D_A(0.3, 1.7)
        D_d = self.cosmo.D_A_z(0.3)
        D_s = self.cosmo.D_A_z(1.7)

        c_Mpc_sec = un.Quantity(c, unit=un.Mpc / un.s)
        G_Mpc3_Msun_sec2 = un.Quantity(G, unit=un.Mpc ** 3 / un.s ** 2 / un.solMass)

        const = c_Mpc_sec ** 2 / (4 * np.pi * G_Mpc3_Msun_sec2)
        sigma_crit_mpc = const.value * D_s / (D_d * D_ds)
        sigma_crit_kpc = sigma_crit_mpc * 1000 ** -2

        npt.assert_almost_equal(self.lens_cosmo.sigma_crit_lensing/sigma_crit_mpc, 1, 4)
        npt.assert_almost_equal(self.lens_cosmo.sigma_crit_lens_kpc/sigma_crit_kpc, 1, 4)

    def test_sigma_crit_mass(self):

        area = 2.
        sigma_crit_mass = self.lens_cosmo.sigma_crit_mass(0.7, area)
        sigma_crit = self.lens_cosmo.get_sigma_crit_lensing(0.7, 1.7)
        npt.assert_almost_equal(sigma_crit_mass, sigma_crit * area)

    def test_colossus(self):

        colossus = self.lens_cosmo.colossus
        npt.assert_almost_equal(colossus.Om0, 0.2)

    def test_truncate_roche(self):

        m = 10**9.
        norm = 1.4
        power = 0.9
        r3d = 1000

        rt = norm * (m / 10 ** 7) ** (1./3) * (r3d / 50) ** power
        rtrunc = self.lens_cosmo.truncation_roche(m, r3d, norm, power)
        npt.assert_almost_equal(rt, rtrunc, 3)

    def test_LOS_trunc(self):

        rt = self.lens_cosmo.LOS_truncation_rN(10**8, 0.2, 90)
        rtrunc = self.lens_cosmo.rN_M_nfw_comoving(10**8 * self.lens_cosmo.cosmo.h, 90, 0.2)
        npt.assert_almost_equal(rt, 1000 * rtrunc * (1+0.2)**-1 / self.lens_cosmo.cosmo.h)

    def test_NFW_concentration(self):

        c = self.lens_cosmo.NFW_concentration(10 ** 9, 0.2, model='diemer19', scatter=False)
        c2 = self.lens_cosmo.NFW_concentration(10 ** 9, 0.2, model='diemer19', scatter=True)
        npt.assert_raises(AssertionError, npt.assert_array_equal, c, c2)

        logmhm = 8.
        kwargs_suppression, suppression_model = {'c_scale': 60., 'c_power': -0.17}, 'polynomial'
        c_wdm = self.lens_cosmo.NFW_concentration(10 ** 9, 0.2, model='diemer19', scatter=False, logmhm=logmhm,
                                                  kwargs_suppresion=kwargs_suppression, suppression_model=suppression_model)

        suppresion = WDM_concentration_suppresion_factor(10**9, 0.2, logmhm, suppression_model, kwargs_suppression)
        npt.assert_almost_equal(suppresion * c, c_wdm)

        kwargs_suppression, suppression_model = {'a_mc': 0.5, 'b_mc': 0.17}, 'hyperbolic'
        c_wdm = self.lens_cosmo.NFW_concentration(10 ** 9, 0.2, model='diemer19', scatter=False, logmhm=logmhm,
                                                  kwargs_suppresion=kwargs_suppression,
                                                  suppression_model=suppression_model)

        suppresion = WDM_concentration_suppresion_factor(10 ** 9, 0.2, logmhm, suppression_model, kwargs_suppression)
        npt.assert_almost_equal(suppresion * c, c_wdm)

    def test_subhalo_accretion(self):

        zi = [self.lens_cosmo.z_accreted_from_zlens(10**8, 0.5)
              for _ in range(0, 20000)]

        h, b = np.histogram(zi, bins=np.linspace(0.5, 6, 20))

        # number at the lens redshift should be about 5x that at redshift 4
        ratio = h[0]/h[12]
        npt.assert_almost_equal(ratio/5 - 1, 0., 1)

    def test_nfw_fundamental_parameters(self):

        for z in [0., 0.74, 1.2]:

            M, c = 10**8, 17.5
            rho_crit_z = self.cosmo.rho_crit(z)

            rhos, rs, r200 = self.lens_cosmo.nfwParam_physical_Mpc(M, c, z)

            h = self.cosmo.h
            _rhos, _rs = self._colossus_nfw.fundamentalParameters(M * h, c, z, '200c')
            # output in units (M h^2 / kpc^2, kpc/h)
            rhos_col = _rhos * h ** 2 * 1000 ** 3
            rs_col = _rs / h / 1000
            r200_col = rs * c

            npt.assert_almost_equal(rhos/rhos_col, 1, 3)
            npt.assert_almost_equal(rs/rs_col, 1, 3)
            npt.assert_almost_equal(r200/r200_col, 1, 3)

            def _profile(x):
                fac = x * (1 + x) ** 2
                return 1. / fac
            def _integrand(x):
                return 4 * np.pi * x ** 2 * _profile(x)

            volume = 4 * np.pi/3 * r200 ** 3
            integral = quad(_integrand, 0, r200/rs)[0]
            mean_density = rhos * rs ** 3 * integral / volume
            ratio = mean_density/rho_crit_z

            npt.assert_almost_equal(ratio/200, 1., 3)

    def test_mhm_convert(self):

        mthermal = 5.3
        mhm = self.lens_cosmo.mthermal_to_halfmode(mthermal)
        mthermal_out = self.lens_cosmo.halfmode_to_thermal(mhm)
        npt.assert_almost_equal(mthermal/mthermal_out, 1, 2)

        fsl = self.lens_cosmo.mhm_to_fsl(10**8.)
        npt.assert_array_less(fsl, 100)

    def test_NFW_phys2angle(self):

        c = self.lens_cosmo.NFW_concentration(10**8, 0.5, scatter=False)
        out = self.lens_cosmo.nfw_physical2angle(10**8, c, 0.5)
        out2 = self.lens_cosmo.nfw_physical2angle_fromM(10**8, 0.5)
        for (x, y) in zip(out, out2):
            npt.assert_almost_equal(x, y)

        rhos_kpc, rs_kpc, _ = self.lens_cosmo.NFW_params_physical(10**8, c, 0.5)
        rhos_mpc = rhos_kpc * 1000 ** 3
        rs_mpc = rs_kpc * 1e-3
        rs, theta_rs = self.lens_cosmo.nfw_physical2angle_fromNFWparams(rhos_mpc, rs_mpc, 0.5)
        npt.assert_almost_equal(rs, out[0])
        npt.assert_almost_equal(theta_rs, out[1])