Source code for lenstronomy.LensModel.Profiles.nie_potential

__author__ = "gipagano"

import numpy as np
import lenstronomy.Util.util as util
import lenstronomy.Util.param_util as param_util
from lenstronomy.LensModel.Profiles.base_profile import LensProfileBase

__all__ = ["NIE_POTENTIAL", "NIEPotentialMajorAxis"]


[docs] class NIE_POTENTIAL(LensProfileBase): """This class implements the elliptical potential of Eq. (67) of `LECTURES ON GRAVITATIONAL LENSING <https://arxiv.org/pdf/astro-ph/9606001.pdf>`_ and Eq. (1) of `Blandford & Kochanek 1987 <http://adsabs.harvard.edu/full/1987ApJ...321..658B>`_, mapped to Eq. (8) of `Barnaka1998 <https://iopscience.iop.org/article/10.1086/305950/fulltext/37798.text.html>`_ to find the ellipticity bounds """ param_names = ["center_x", "center_y", "theta_E", "theta_c", "e1", "e2"] lower_limit_default = { "center_x": -100, "center_y": -100, "theta_E": 0, "theta_c": 0, "e1": 0, "e2": 0, } upper_limit_default = { "center_x": 100, "center_y": 100, "theta_E": 10, "theta_c": 10, "e1": 0.2, "e2": 0.2, }
[docs] def __init__(self): self.nie_potential_major_axis = NIEPotentialMajorAxis() super(NIE_POTENTIAL, self).__init__()
[docs] def param_conv(self, theta_E, theta_c, e1, e2): if self._static is True: return ( self._thetaE_transf_static, self._thetac_static, self._eps_static, self._phi_G_static, ) return self._param_conv(theta_E, theta_c, e1, e2)
def _param_conv(self, theta_E, theta_c, e1, e2): """Convert the spherical averaged Einstein radius to an elliptical (major axis) Einstein radius and the individual eccentricities to the modulus of the eccentricity. :param theta_E: Einstein radius :param theta_c: core radius :param e1: eccentricity component :param e2: eccentricity component :return: transformed Einstein radius, core radius, ellipticity modulus, orientation angle phi_G """ eps = np.sqrt(e1**2 + e2**2) phi_G, q = param_util.ellipticity2phi_q(e1, e2) theta_E_conv = self._theta_q_convert(theta_E, q) theta_c_conv = self._theta_q_convert(theta_c, q) return theta_E_conv, theta_c_conv, eps, phi_G
[docs] def set_static(self, theta_E, theta_c, e1, e2, center_x=0, center_y=0): """ :param x: x-coordinate in image plane :param y: y-coordinate in image plane :param theta_E: Einstein radius :param theta_c: core radius :param e1: eccentricity component :param e2: eccentricity component :param center_x: profile center :param center_y: profile center :return: self variables set """ self._static = True ( self._thetaE_transf_static, self._thetac_static, self._eps_static, self._phi_G_static, ) = self._param_conv(theta_E, theta_c, e1, e2)
[docs] def set_dynamic(self): """ :return: """ self._static = False if hasattr(self, "_thetaE_transf_static"): del self._thetaE_transf_static if hasattr(self, "_thetac_static"): del self._thetac_static if hasattr(self, "_eps_static"): del self._eps_static if hasattr(self, "_phi_G_static"): del self._phi_G_static
[docs] def function(self, x, y, theta_E, theta_c, e1, e2, center_x=0, center_y=0): """ :param x: x-coord (in angles) :param y: y-coord (in angles) :param theta_E: Einstein radius (in angles) :param theta_c: core radius (in angles) :param e1: eccentricity component, x direction(dimensionless) :param e2: eccentricity component, y direction (dimensionless) :return: lensing potential """ theta_E_conv, theta_c_conv, eps, phi_G = self.param_conv( theta_E, theta_c, e1, e2 ) # shift x_ = x - center_x y_ = y - center_y # rotate x__, y__ = util.rotate(x_, y_, phi_G) # evaluate f_ = self.nie_potential_major_axis.function( x__, y__, theta_E_conv, theta_c_conv, eps ) # rotate back return f_
[docs] def derivatives(self, x, y, theta_E, theta_c, e1, e2, center_x=0, center_y=0): """ :param x: x-coord (in angles) :param y: y-coord (in angles) :param theta_E: Einstein radius (in angles) :param theta_c: core radius (in angles) :param e1: eccentricity component, x direction(dimensionless) :param e2: eccentricity component, y direction (dimensionless) :return: deflection angle (in angles) """ theta_E_conv, theta_c_conv, eps, phi_G = self.param_conv( theta_E, theta_c, e1, e2 ) # shift x_ = x - center_x y_ = y - center_y # rotate x__, y__ = util.rotate(x_, y_, phi_G) # evaluate f__x, f__y = self.nie_potential_major_axis.derivatives( x__, y__, theta_E_conv, theta_c_conv, eps ) # rotate back f_x, f_y = util.rotate(f__x, f__y, -phi_G) return f_x, f_y
[docs] def hessian(self, x, y, theta_E, theta_c, e1, e2, center_x=0, center_y=0): """ :param x: x-coord (in angles) :param y: y-coord (in angles) :param theta_E: Einstein radius (in angles) :param theta_c: core radius (in angles) :param e1: eccentricity component, x direction(dimensionless) :param e2: eccentricity component, y direction (dimensionless) :return: hessian matrix (in angles) """ theta_E_conv, theta_c_conv, eps, phi_G = self.param_conv( theta_E, theta_c, e1, e2 ) # shift x_ = x - center_x y_ = y - center_y # rotate x__, y__ = util.rotate(x_, y_, phi_G) # evaluate f__xx, f__xy, _, f__yy = self.nie_potential_major_axis.hessian( x__, y__, theta_E_conv, theta_c_conv, eps ) # rotate back kappa = 1.0 / 2 * (f__xx + f__yy) gamma1__ = 1.0 / 2 * (f__xx - f__yy) gamma2__ = f__xy gamma1 = np.cos(2 * phi_G) * gamma1__ - np.sin(2 * phi_G) * gamma2__ gamma2 = +np.sin(2 * phi_G) * gamma1__ + np.cos(2 * phi_G) * gamma2__ f_xx = kappa + gamma1 f_yy = kappa - gamma1 f_xy = gamma2 return f_xx, f_xy, f_xy, f_yy
def _theta_q_convert(self, theta_E, q): """Converts a spherical averaged Einstein radius/core radius to an elliptical (major axis) Einstein radius. This then follows the convention of the SPEMD profile in lenstronomy. (theta_E / theta_E_gravlens) = sqrt[ (1+q^2) / (2 q) ] :param theta_E: Einstein radius in lenstronomy conventions :param q: axis ratio minor/major :return: theta_E in convention of kappa= b *(q2(s2 + x2) + y2􏰉)−1/2 """ theta_E_new = theta_E / (np.sqrt((1.0 + q**2) / (2.0 * q))) # / (1+(1-q)/2.) return theta_E_new
[docs] class NIEPotentialMajorAxis(LensProfileBase): """This class implements the elliptical potential of Eq. (67) of `LECTURES ON GRAVITATIONAL LENSING <https://arxiv.org/pdf/astro-ph/9606001.pdf>`_ and Eq. (1) of `Blandford & Kochanek 1987 <http://adsabs.harvard.edu/full/1987ApJ...321..658B>`_, mapped to Eq. (8) of `Barnaka1998 <https://iopscience.iop.org/article/10.1086/305950/fulltext/37798.text.html>`_ to find the ellipticity bounds """ param_names = ["theta_E", "theta_c", "eps", "center_x", "center_y"]
[docs] def __init__(self, diff=0.0000000001): self._diff = diff super(NIEPotentialMajorAxis, self).__init__()
[docs] def function(self, x, y, theta_E, theta_c, eps): f_ = theta_E * np.sqrt(theta_c**2 + (1 - eps) * x**2 + (1 + eps) * y**2) return f_
[docs] def derivatives(self, x, y, theta_E, theta_c, eps): """Returns df/dx and df/dy of the function.""" factor = np.sqrt(theta_c**2 + (1 - eps) * x**2 + (1 + eps) * y**2) f_x = (theta_E / factor) * (1 - eps) * x f_y = (theta_E / factor) * (1 + eps) * y return f_x, f_y
[docs] def hessian(self, x, y, theta_E, theta_c, eps): """Returns Hessian matrix of function d^2f/dx^2, d^2/dxdy, d^2/dydx, d^f/dy^2.""" factor = np.sqrt(theta_c**2 + (1 - eps) * x**2 + (1 + eps) * y**2) f_xx = (1 - eps) * (theta_E / factor) - (theta_E / factor**3) * ( 1 - eps ) ** 2 * x**2 f_yy = (1 + eps) * (theta_E / factor) - (theta_E / factor**3) * ( 1 + eps ) ** 2 * y**2 f_xy = -(theta_E / factor**3) * (1 - eps**2) * x * y return f_xx, f_xy, f_xy, f_yy