Python scipy.empty_like函数代码示例

 def density_2s(self, n1, n2):
     """Returns a reduced density matrix for a pair of sites.
     
     Parameters
     ----------
     n1 : int
         The site number of the first site.
     n2 : int
         The site number of the second site (must be > n1).        
     """
     rho = sp.empty((self.q[n1] * self.q[n2], self.q[n1] * self.q[n2]), dtype=sp.complex128)
     r_n2 = sp.empty_like(self.r[n2 - 1])
     r_n1 = sp.empty_like(self.r[n1 - 1])
     
     for s2 in xrange(self.q[n2]):
         for t2 in xrange(self.q[n2]):
             r_n2 = m.mmul(self.A[n2][t2], self.r[n2], m.H(self.A[n2][s2]))
             
             r_n = r_n2
             for n in reversed(xrange(n1 + 1, n2)):
                 r_n = self.eps_r(n, r_n)        
                 
             for s1 in xrange(self.q[n1]):
                 for t1 in xrange(self.q[n1]):
                     r_n1 = m.mmul(self.A[n1][t1], r_n, m.H(self.A[n1][s1]))
                     tmp = m.mmul(self.l[n1 - 1], r_n1)
                     rho[s1 * self.q[n1] + s2, t1 * self.q[n1] + t2] = tmp.trace()
     return rho

    def density_2s(self, n1, n2):
        """Returns a reduced density matrix for a pair of sites.
        
        Currently only supports sites in the nonuniform window.

        Parameters
        ----------
        n1 : int
            The site number of the first site.
        n2 : int
            The site number of the second site (must be > n1).
        """
        rho = sp.empty((self.q[n1] * self.q[n2], self.q[n1] * self.q[n2]), dtype=sp.complex128)
        r_n2 = sp.empty_like(self.r[n2 - 1])
        r_n1 = sp.empty_like(self.r[n1 - 1])
        ln1m1 = self.get_l(n1 - 1)

        for s2 in xrange(self.q[n2]):
            for t2 in xrange(self.q[n2]):
                r_n2 = mm.mmul(self.A[n2][t2], self.r[n2], mm.H(self.A[n2][s2]))

                r_n = r_n2
                for n in reversed(xrange(n1 + 1, n2)):
                    r_n = tm.eps_r_noop(r_n, self.A[n], self.A[n])

                for s1 in xrange(self.q[n1]):
                    for t1 in xrange(self.q[n1]):
                        r_n1 = mm.mmul(self.A[n1][t1], r_n, mm.H(self.A[n1][s1]))
                        tmp = mm.adot(ln1m1, r_n1)
                        rho[s1 * self.q[n1] + s2, t1 * self.q[n1] + t2] = tmp
        return rho

 def calc_x(self, n, Vsh, sqrt_l, sqrt_r, sqrt_l_inv, sqrt_r_inv):
     """Calculate the parameter matrix x* giving the desired B.
     
     This is equivalent to eqn. (49) of arXiv:1103.0936v2 [cond-mat.str-el] except 
     that, here, norm-preservation is not enforced, such that the optimal 
     parameter matrices x*_n (for the parametrization of B) are given by the 
     derivative w.r.t. x_n of <Phi[B, A]|Ĥ|Psi[A]>, rather than 
     <Phi[B, A]|Ĥ - H|Psi[A]> (with H = <Psi|Ĥ|Psi>).
     
     An additional sum was added for the single-site hamiltonian.
     
     Some multiplications have been pulled outside of the sums for efficiency.
     
     Direct dependencies: 
         - A[n - 1], A[n], A[n + 1]
         - r[n], r[n + 1], l[n - 2], l[n - 1]
         - C[n], C[n - 1]
         - K[n + 1]
         - V[n]
     """
     x = sp.zeros((self.D[n - 1], self.q[n] * self.D[n] - self.D[n - 1]), dtype=self.typ, order=self.odr)
     x_part = sp.empty_like(x)
     x_subpart = sp.empty_like(self.A[n][0])
     x_subsubpart = sp.empty_like(self.A[n][0])
     
     x_part.fill(0)
     for s in xrange(self.q[n]):
         x_subpart.fill(0)    
         
         if n < self.N:
             x_subsubpart.fill(0)
             for t in xrange(self.q[n + 1]):
                 x_subsubpart += m.mmul(self.C[n][s,t], self.r[n + 1], m.H(self.A[n + 1][t])) #~1st line
                 
             x_subsubpart += m.mmul(self.A[n][s], self.K[n + 1]) #~3rd line               
             
             x_subpart += m.mmul(x_subsubpart, sqrt_r_inv)
         
         if not self.h_ext is None:
             x_subsubpart.fill(0)
             for t in xrange(self.q[n]):                         #Extra term to take care of h_ext..
                 x_subsubpart += self.h_ext(n, s, t) * self.A[n][t] #it may be more effecient to squeeze this into the nn term...
             x_subpart += m.mmul(x_subsubpart, sqrt_r)
         
         x_part += m.mmul(x_subpart, Vsh[s])
             
     x += m.mmul(sqrt_l, x_part)
         
     if n > 1:
         x_part.fill(0)
         for s in xrange(self.q[n]):     #~2nd line
             x_subsubpart.fill(0)
             for t in xrange(self.q[n + 1]):
                 x_subsubpart += m.mmul(m.H(self.A[n - 1][t]), self.l[n - 2], self.C[n - 1][t, s])
             x_part += m.mmul(x_subsubpart, sqrt_r, Vsh[s])
         x += m.mmul(sqrt_l_inv, x_part)
             
     return x

def shifted_matrix_sub(data, sub, tau, pad_val=0.0):
    """Subtracts the multi-channeled vector (rows are channels) y from
    the vector x with a certain offset. x and y can due to the offset be only
    partly overlapping.

    REM: from matlab

    :type data: ndarray
    :param data: data array to apply the subtractor to
    :type sub: ndarray
    :param sub: subtractor array
    :type tau: int
    :param tau: offset of :sub: w.r.t. start of :data:
    :type pad_val: float
    :param pad_val: value to use for the padding
        Default=0.0
    :return: ndarray - data minus sub at offset, len(data)
    """

    ns_data, nc_data = data.shape
    ns_sub, nc_sub = sub.shape
    if nc_data != nc_sub:
        raise ValueError('nc_data and nc_sub must agree!')
    tau = int(tau)
    data_sub = sp.empty_like(data)
    data_sub[:] = pad_val
    data_sub[max(0, tau):tau + ns_sub] = sub[max(0, -tau):ns_data - tau]
    return data - data_sub

def dispersion_relation_extraordinary(kx, ky, k, nO, nE, c):
    """Dispersion relation for the extraordinary wave.

    NOTE
    See eq. 16 in Glytsis, "Three-dimensional (vector) rigorous
    coupled-wave analysis of anisotropic grating diffraction",
    JOSA A, 7(8), 1990 Always give positive real or negative
    imaginary.
    """

    if kx.shape != ky.shape or c.size != 3:
        raise ValueError('kx and ky must have the same length and c must have 3 components')

    kz = S.empty_like(kx)

    for ii in xrange(0, kx.size):

        alpha = nE**2 - nO**2
        beta = kx[ii]/k * c[0] + ky[ii]/k * c[1]

        # coeffs
        C = S.array([nO**2 + c[2]**2 * alpha, \
                     2. * c[2] * beta * alpha, \
                     nO**2 * (kx[ii]**2 + ky[ii]**2) / k**2 + alpha * beta**2 - nO**2 * nE**2])

        # two solutions of type +x or -x, purely real or purely imag
        tmp_kz = k * S.roots(C)

        # get the negative imaginary part or the positive real one
        if S.any(S.isreal(tmp_kz)):
            kz[ii] = S.absolute(tmp_kz[0])
        else:
            kz[ii] = -1j * S.absolute(tmp_kz[0])

    return kz

    def predict_proba(self, X):
        """
        Predict the membership probabilities for the data samples
        in X using trained model.

        Parameters
        ----------
        X : array-like, shape (n_samples, n_features)
            List of n_features-dimensional data points. Each row
            corresponds to a single data point.

        Returns
        -------
        proba : array, shape (n_samples, n_clusters)
        """
        X = check_array(X, copy=False, order='C', dtype=sp.float64)
        K = self.score_samples(X)
        T = sp.empty_like(K)

        # Compute the Loglikelhood
        K *= (0.5)

        # Compute the posterior
        with sp.errstate(over='ignore'):
            for c in xrange(self.C):
                T[:, c] = 1 / sp.exp(K-K[:, c][:, sp.newaxis]).sum(axis=1)

        return T

 def scale(self,x,M=None,m=None):  # TODO:  DO IN PLACE SCALING
     """[email protected] Function that standardize the data
     
         Input:
             x: the data
             M: the Max vector
             m: the Min vector
         Output:
             x: the standardize data
             M: the Max vector
             m: the Min vector
     """
     [n,d]=x.shape
     if not sp.issubdtype(x.dtype,float):
         x=x.astype('float')
 
     # Initialization of the output
     xs = sp.empty_like(x)
 
     # get the parameters of the scaling
     if M is None:
         M,m = sp.amax(x,axis=0),sp.amin(x,axis=0)
         
     den = M-m
     for i in range(d):
         if den[i] != 0:
             xs[:,i] = 2*(x[:,i]-m[i])/den[i]-1
         else:
             xs[:,i]=x[:,i]
 
     return xs

    def calc_B(self, n, set_eta=True):
        """Generates the B[n] tangent vector corresponding to physical evolution of the state.

        In other words, this returns B[n][x*] (equiv. eqn. (47) of
        arXiv:1103.0936v2 [cond-mat.str-el])
        with x* the parameter matrices satisfying the Euler-Lagrange equations
        as closely as possible.
        
        In the case of Bc, use the general Bc generated in calc_B_centre().
        """
        if n == self.N_centre:
            B, eta_sq_c = self.calc_B_centre()
            if set_eta:
                self.eta_sq[self.N_centre] = eta_sq_c
        else:
            l_sqrt, r_sqrt, l_sqrt_inv, r_sqrt_inv = self.calc_l_r_roots(n)
            
            if n > self.N_centre:
                Vsh = tm.calc_Vsh(self.A[n], r_sqrt, sanity_checks=self.sanity_checks)
                x = self.calc_x(n, Vsh, l_sqrt, r_sqrt, l_sqrt_inv, r_sqrt_inv, right=True)
                
                B = sp.empty_like(self.A[n])
                for s in range(self.q[n]):
                    B[s] = mm.mmul(l_sqrt_inv, x, mm.H(Vsh[s]), r_sqrt_inv)
                    
                if self.sanity_checks:
                    M = tm.eps_r_noop(self.r[n], B, self.A[n])
                    if not sp.allclose(M, 0):
                        print("Sanity Fail in calc_B!: B_%u does not satisfy GFC!" % n)
            else:
                Vsh = tm.calc_Vsh_l(self.A[n], l_sqrt, sanity_checks=self.sanity_checks)
                x = self.calc_x(n, Vsh, l_sqrt, r_sqrt, l_sqrt_inv, r_sqrt_inv, right=False)
                
                B = sp.empty_like(self.A[n])
                for s in range(self.q[n]):
                    B[s] = mm.mmul(l_sqrt_inv, mm.H(Vsh[s]), x, r_sqrt_inv)
                    
                if self.sanity_checks:
                    M = tm.eps_l_noop(self.l[n - 1], B, self.A[n])
                    if not sp.allclose(M, 0):
                        print("Sanity Fail in calc_B!: B_%u does not satisfy GFC!" % n)
            
            if set_eta:
                self.eta_sq[n] = mm.adot(x, x)


        return B

 def calc_B1(self):
     """Calculate the optimal B1 given right gauge-fixing on B2..N and
     no gauge-fixing on B1.
     
     We use the non-norm-preserving K's, since the norm-preservation
     is not needed elsewhere. It is cleaner to subtract the relevant
     norm-changing terms from the K's here than to generate all K's
     with norm-preservation.
     """
     B1 = sp.empty_like(self.A[1])
     
     try:
         r1_i = self.r[1].inv()
     except AttributeError:
         r1_i = mm.invmh(self.r[1])
         
     try:
         l0_i = self.l[0].inv()
     except AttributeError:
         l0_i = mm.invmh(self.l[0])
     
     A0 = self.A[0]
     A1 = self.A[1]
     A2 = self.A[2]
     r1 = self.r[1]
     r2 = self.r[2]
     l0 = self.l[0]
     
     KLh = mm.H(self.u_gnd_l.K_left - l0 * mm.adot(self.u_gnd_l.K_left, self.r[0]))
     K2 = self.K[2] - r1 * mm.adot(self.l[1], self.K[2])
     
     C1 = self.C[1] - self.h_expect[1] * self.AA1
     C0 = self.C[0] - self.h_expect[0] * self.AA0
     
     for s in xrange(self.q[1]):
         try:
             B1[s] = A1[s].dot(r1_i.dot_left(K2))
         except AttributeError:
             B1[s] = A1[s].dot(K2.dot(r1_i))
         
         for t in xrange(self.q[2]):
             try:
                 B1[s] += C1[s, t].dot(r2.dot(r1_i.dot_left(mm.H(A2[t]))))
             except AttributeError:
                 B1[s] += C1[s, t].dot(r2.dot(mm.H(A2[t]).dot(r1_i)))                    
             
         B1sbit = KLh.dot(A1[s])
                         
         for t in xrange(self.q[0]):
             B1sbit += mm.H(A0[t]).dot(l0.dot(C0[t,s]))
             
         B1[s] += l0_i.dot(B1sbit)
        
     rb = sp.zeros_like(self.r[0])
     for s in xrange(self.q[1]):
         rb += B1[s].dot(r1.dot(mm.H(B1[s])))
     eta = sp.sqrt(mm.adot(l0, rb))
             
     return B1, eta

def calculate_slow_phi_0s(phi_0s, p_values):
    slow_phi_0s = scipy.empty_like(phi_0s)
    for i, phi_0 in enumerate(phi_0s):
        phi_0_unfolded = unfold(phi_0)
        x = arange(len(phi_0_unfolded))
        model = polyfit(x, phi_0_unfolded, 3, w=p_values[i])
        slow_phi_0s[i] = polyval(model, x)
    return slow_phi_0s

    def calc_C(self, n_low=-1, n_high=-1):
        """Generates the C matrices used to calculate the K's and ultimately the B's

        These are to be used on one side of the super-operator when applying the
        nearest-neighbour Hamiltonian, similarly to C in eqn. (44) of
        arXiv:1103.0936v2 [cond-mat.str-el], except being for the non-norm-preserving case.

        Makes use only of the nearest-neighbour hamiltonian, and of the A's.

        C[n] depends on A[n] and A[n + 1].
        
        This calculation can be significantly faster if a matrix form for h_nn
        is available. See gen_h_matrix().

        """
        if self.h_nn is None:
            return 0

        if n_low < 1:
            n_low = 0
        if n_high < 1:
            n_high = self.N + 1
        
        if self.h_nn_mat is None:
            for n in xrange(n_low, n_high):
                self.C[n].fill(0)
                for u in xrange(self.q[n]):
                    for v in xrange(self.q[n + 1]):
                        AA = mm.mmul(self.A[n][u], self.A[n + 1][v]) #only do this once for each
                        for s in xrange(self.q[n]):
                            for t in xrange(self.q[n + 1]):
                                h_nn_stuv = self.h_nn(n, s, t, u, v)
                                if h_nn_stuv != 0:
                                    self.C[n][s, t] += h_nn_stuv * AA
        else:
            dot = sp.dot
            for n in xrange(n_low, n_high):
                An = self.A[n]
                Anp1 = self.A[n + 1]
                
                AA = sp.empty_like(self.C[n])
                for u in xrange(self.q[n]):
                    for v in xrange(self.q[n + 1]):
                        AA[u, v] = dot(An[u], Anp1[v])
                        
                if n == 0: #FIXME: Temp. hack
                    self.AA0 = AA
                elif n == 1:
                    self.AA1 = AA
                
                res = sp.tensordot(AA, self.h_nn_mat[n], ((0, 1), (2, 3)))
                res = sp.rollaxis(res, 3)
                res = sp.rollaxis(res, 3)
                
                self.C[n][:] = res

def oppwalker_convert(arr):
    #assert(arr.min()>=0 and arr.max()<=1)
    out = sp.empty_like(arr)

    # red-green
    out[:,:,0] = arr[:,:,0] - arr[:,:,1]
    # blue-yellow
    out[:,:,1] = arr[:,:,2] - arr[:,:,[0,1]].min(2)
    # intensity
    out[:,:,2] = arr.max(2)

    return out

def BiotLineIntegral(vect_arr, r_p, current=1.0):
    """
    Calculates the magnetic flux density of from a list of points
    (vect_arr) that represent a discretization of a conductor.
    The magnetic flux density is calculated for r_p positions.
    
    Parameters
    ----------
    vect_arr: array([[x_0,y_0,z_0], ... , [x_n,y_n,z_n]])
    r_p: array([[x_0,y_0,z_0], ... , [x_n,y_n,z_n]])

    All coordinates are in mm

    Returns
    ----------
    Magnetric flux density Bfield, same as r_p
    
    """
    bfield = scipy.empty_like(r_p, scipy.float64)
    code = """
    #include <iostream>
    #include <math.h>
    #include <assert.h>
    for(int ir_p = 0; ir_p < size_r_p; ir_p++) {
        vec3 wire_pre = { vect_arr(0,0), vect_arr(0,1), vect_arr(0,2) };
        vec3 bfield_vec = { 0.0, 0.0, 0.0 };
        vec3 vec3r_p = { r_p(ir_p, 0), r_p(ir_p, 1), r_p(ir_p, 2) };  
        for(int i_v  = 1; i_v < size_vect_arr; i_v++) {
            vec3 vec3_arr = { vect_arr(i_v,0), vect_arr(i_v,1), vect_arr(i_v,2) };
            vec3 dl = vec3_diff( vec3_arr, wire_pre);
            vec3 rs = vec3_arr;
            vec3 r  = vec3_diff( vec3r_p, rs );
            double r_length = vec3_abs(r);
            bfield_vec      =  vec3_add( vec3_scale( vec3_cross( dl, r), 1.0 / pow( r_length, 3)), bfield_vec );
            wire_pre        = vec3_arr;
        }
        bfield(ir_p, 0) = bfield_vec.x ;
        bfield(ir_p, 1) = bfield_vec.y ;
        bfield(ir_p, 2) = bfield_vec.z ;
    }
    return_val = 1;
    """
    size_r_p          = r_p[:, 0].size
    size_vect_arr     = vect_arr[:, 0].size
    os.path.realpath(__file__)
    support_code = open( os.path.dirname(__file__) + "/biot_blitz_support.cpp" )
    scipy.weave.inline(code,
                       ["r_p", "size_r_p", "bfield", "vect_arr", "size_vect_arr"],
                       type_converters=converters.blitz,
                       support_code=support_code.read(),
                       compiler='gcc' )
    return bfield * mu_0 * 1000.0 * 1.0/(4.0 * pi)

def oppsande_convert(arr):
    #assert(arr.min()>=0 and arr.max()<=1)

    r = arr[:,:,0]
    g = arr[:,:,1]
    b = arr[:,:,2]
    
    out = sp.empty_like(arr)
    out[:,:,0] = (r-g) / sp.sqrt(2.)
    out[:,:,1] = (r+g-2.*b) / sp.sqrt(6.)
    out[:,:,2] = (r+g+b) / sp.sqrt(3.)

    return out

def invE_convert(arr):
    #assert(arr.min()>=0 and arr.max()<=1)
    
    red = arr[:,:,0]
    green = arr[:,:,1]
    blue = arr[:,:,2]

    out = sp.empty_like(arr)

    out[:,:,0] = (red + green + blue) / 3.
    out[:,:,1] = (red + green - 2.*blue) / 4.
    out[:,:,2] = (red - 2.*green + blue) / 4.

    return out