示例#1
0
def get_param(par, args, m1, m2, s1z, s2z):
    """
    Helper function

    Parameters
    ----------
    par : string
        Name of parameter to calculate
    args : Namespace object returned from ArgumentParser instance
        Calling code command line options, used for f_lower value
    m1 : float or array of floats
        First binary component mass (etc.)

    Returns
    -------
    parvals : float or array of floats
        Calculated parameter values
    """
    if par == 'mchirp':
        parvals, _ = pnutils.mass1_mass2_to_mchirp_eta(m1, m2)
    elif par == 'mtotal':
        parvals = m1 + m2
    elif par == 'template_duration':
        # default to SEOBNRv4 duration function
        parvals = pnutils.get_imr_duration(m1, m2, s1z, s2z, args.f_lower,
                                           args.approximant or "SEOBNRv4")
        if args.min_duration:
            parvals += args.min_duration
    elif par in pnutils.named_frequency_cutoffs.keys():
        parvals = pnutils.frequency_cutoff_from_name(par, m1, m2, s1z, s2z)
    else:
        # try asking for a LALSimulation frequency function
        parvals = pnutils.get_freq(par, m1, m2, s1z, s2z)
    return parvals
示例#2
0
def get_param(par, args, m1, m2, s1z, s2z):
    """
    Helper function

    Parameters
    ----------
    par : string
        Name of parameter to calculate
    args : Namespace object returned from ArgumentParser instance
        Calling code command line options, used for f_lower value
    m1 : float or array of floats
        First binary component mass (etc.)

    Returns
    -------
    parvals : float or array of floats
        Calculated parameter values
    """
    if par == 'mchirp':
        parvals, _ = pnutils.mass1_mass2_to_mchirp_eta(m1, m2)
    elif par == 'mtotal':
        parvals = m1 + m2
    elif par == 'template_duration':
        # default to SEOBNRv4 duration function
        parvals = pnutils.get_imr_duration(m1, m2, s1z, s2z, args.f_lower,
                                           args.approximant or "SEOBNRv4")
        if args.min_duration:
            parvals += args.min_duration
    elif par in pnutils.named_frequency_cutoffs.keys():
        parvals = pnutils.frequency_cutoff_from_name(par, m1, m2, s1z, s2z)
    else:
        # try asking for a LALSimulation frequency function
        parvals = pnutils.get_freq(par, m1, m2, s1z, s2z)
    return parvals
示例#3
0
文件: triggers.py 项目: cmbiwer/pycbc
def get_param(par, args, m1, m2, s1z, s2z):
    """
    Helper function

    Parameters
    ----------
    par : string
        Name of parameter to calculate
    args : Namespace object returned from ArgumentParser instance
        Calling code command line options, used for f_lower value
    m1 : float or array of floats
        First binary component mass (etc.)

    Returns
    -------
    parvals : float or array of floats
        Calculated parameter values
    """
    if par == 'mchirp':
        parvals = conversions.mchirp_from_mass1_mass2(m1, m2)
    elif par == 'mtotal':
        parvals = m1 + m2
    elif par == 'eta':
        parvals = conversions.eta_from_mass1_mass2(m1, m2)
    elif par in ['chi_eff', 'effective_spin']:
        parvals = conversions.chi_eff(m1, m2, s1z, s2z)
    elif par == 'template_duration':
        # default to SEOBNRv4 duration function
        if not hasattr(args, 'approximant') or args.approximant is None:
            args.approximant = "SEOBNRv4"
        parvals = pnutils.get_imr_duration(m1, m2, s1z, s2z, args.f_lower,
                                           args.approximant)
        if args.min_duration:
            parvals += args.min_duration
    elif par == 'tau0':
        parvals = conversions.tau0_from_mass1_mass2(m1, m2, args.f_lower)
    elif par == 'tau3':
        parvals = conversions.tau3_from_mass1_mass2(m1, m2, args.f_lower)
    elif par in pnutils.named_frequency_cutoffs.keys():
        parvals = pnutils.frequency_cutoff_from_name(par, m1, m2, s1z, s2z)
    else:
        # try asking for a LALSimulation frequency function
        parvals = pnutils.get_freq(par, m1, m2, s1z, s2z)
    return parvals
示例#4
0
def output_sngl_inspiral_table(outputFile,
                               tempBank,
                               metricParams,
                               ethincaParams,
                               programName="",
                               optDict=None,
                               outdoc=None,
                               **kwargs):
    """
    Function that converts the information produced by the various pyCBC bank
    generation codes into a valid LIGOLW xml file containing a sngl_inspiral
    table and outputs to file.
 
    Parameters
    -----------
    outputFile : string
        Name of the file that the bank will be written to
    tempBank : iterable
        Each entry in the tempBank iterable should be a sequence of
        [mass1,mass2,spin1z,spin2z] in that order.
    metricParams : metricParameters instance
        Structure holding all the options for construction of the metric
        and the eigenvalues, eigenvectors and covariance matrix
        needed to manipulate the space.
    ethincaParams: {ethincaParameters instance, None}
        Structure holding options relevant to the ethinca metric computation
        including the upper frequency cutoff to be used for filtering.
        NOTE: The computation is currently only valid for non-spinning systems
        and uses the TaylorF2 approximant.
    programName (key-word-argument) : string
        Name of the executable that has been run
    optDict (key-word argument) : dictionary
        Dictionary of the command line arguments passed to the program
    outdoc (key-word argument) : ligolw xml document
        If given add template bank to this representation of a xml document and
        write to disk. If not given create a new document.
    kwargs : key-word arguments
        All other key word arguments will be passed directly to 
        ligolw_process.register_to_xmldoc
    """
    if optDict is None:
        optDict = {}
    if outdoc is None:
        outdoc = ligolw.Document()
        outdoc.appendChild(ligolw.LIGO_LW())

    # get IFO to put in search summary table
    ifos = []
    if 'channel_name' in optDict.keys():
        if optDict['channel_name'] is not None:
            ifos = [optDict['channel_name'][0:2]]

    proc_id = ligolw_process.register_to_xmldoc(outdoc,
                                                programName,
                                                optDict,
                                                ifos=ifos,
                                                **kwargs).process_id
    sngl_inspiral_table = convert_to_sngl_inspiral_table(tempBank, proc_id)
    # Calculate Gamma components if needed
    if ethincaParams is not None:
        if ethincaParams.doEthinca:
            for sngl in sngl_inspiral_table:
                # Set tau_0 and tau_3 values needed for the calculation of
                # ethinca metric distances
                (sngl.tau0, sngl.tau3) = pnutils.mass1_mass2_to_tau0_tau3(
                    sngl.mass1, sngl.mass2, metricParams.f0)
                fMax_theor, GammaVals = calculate_ethinca_metric_comps(
                    metricParams,
                    ethincaParams,
                    sngl.mass1,
                    sngl.mass2,
                    spin1z=sngl.spin1z,
                    spin2z=sngl.spin2z,
                    full_ethinca=ethincaParams.full_ethinca)
                # assign the upper frequency cutoff and Gamma0-5 values
                sngl.f_final = fMax_theor
                for i in xrange(len(GammaVals)):
                    setattr(sngl, "Gamma" + str(i), GammaVals[i])
        # If Gamma metric components are not wanted, assign f_final from an
        # upper frequency cutoff specified in ethincaParams
        elif ethincaParams.cutoff is not None:
            for sngl in sngl_inspiral_table:
                sngl.f_final = pnutils.frequency_cutoff_from_name(
                    ethincaParams.cutoff, sngl.mass1, sngl.mass2, sngl.spin1z,
                    sngl.spin2z)

    # set per-template low-frequency cutoff
    if 'f_low_column' in optDict and 'f_low' in optDict and \
            optDict['f_low_column'] is not None:
        for sngl in sngl_inspiral_table:
            setattr(sngl, optDict['f_low_column'], optDict['f_low'])

    outdoc.childNodes[0].appendChild(sngl_inspiral_table)

    # get times to put in search summary table
    start_time = 0
    end_time = 0
    if 'gps_start_time' in optDict.keys() and 'gps_end_time' in optDict.keys():
        start_time = optDict['gps_start_time']
        end_time = optDict['gps_end_time']

    # make search summary table
    search_summary_table = lsctables.New(lsctables.SearchSummaryTable)
    search_summary = return_search_summary(start_time, end_time,
                                           len(sngl_inspiral_table), ifos,
                                           **kwargs)
    search_summary_table.append(search_summary)
    outdoc.childNodes[0].appendChild(search_summary_table)

    # write the xml doc to disk
    proctable = table.get_table(outdoc, lsctables.ProcessTable.tableName)
    ligolw_utils.write_filename(outdoc,
                                outputFile,
                                gz=outputFile.endswith('.gz'))
示例#5
0
def calculate_ethinca_metric_comps(metricParams,
                                   ethincaParams,
                                   mass1,
                                   mass2,
                                   spin1z=0.,
                                   spin2z=0.,
                                   full_ethinca=True):
    """
    Calculate the Gamma components needed to use the ethinca metric.
    At present this outputs the standard TaylorF2 metric over the end time 
    and chirp times \tau_0 and \tau_3.
    A desirable upgrade might be to use the \chi coordinates [defined WHERE?] 
    for metric distance instead of \tau_0 and \tau_3.
    The lower frequency cutoff is currently hard-coded to be the same as the 
    bank layout options fLow and f0 (which must be the same as each other).

    Parameters
    -----------
    metricParams : metricParameters instance
        Structure holding all the options for construction of the metric
        and the eigenvalues, eigenvectors and covariance matrix
        needed to manipulate the space.
    ethincaParams : ethincaParameters instance
        Structure holding options relevant to the ethinca metric computation.
    mass1 : float
        Mass of the heavier body in the considered template.
    mass2 : float
        Mass of the lighter body in the considered template.
    spin1z : float (optional, default=0)
        Spin of the heavier body in the considered template.
    spin2z : float (optional, default=0)
        Spin of the lighter body in the considered template.
    full_ethinca : boolean (optional, default=True)
        If True calculate the ethinca components in all 3 directions (mass1,
        mass2 and time). If False calculate only the time component (which is
        stored in Gamma0).
    Returns
    --------
    fMax_theor : float
        Value of the upper frequency cutoff given by the template parameters
        and the cutoff formula requested.

    gammaVals : numpy_array
        Array holding 6 independent metric components in 
        (end_time, tau_0, tau_3) coordinates to be stored in the Gamma0-5 
        slots of a SnglInspiral object.
    """
    if (float(spin1z) != 0. or float(spin2z) != 0.) and full_ethinca:
        raise NotImplementedError("Ethinca cannot at present be calculated "
                                  "for nonzero component spins!")
    f0 = metricParams.f0
    if f0 != metricParams.fLow:
        raise ValueError("If calculating ethinca the bank f0 value must be "
                         "equal to f-low!")
    if ethincaParams.fLow is not None and (ethincaParams.fLow !=
                                           metricParams.fLow):
        raise NotImplementedError("An ethinca metric f-low different from the"
                                  " bank metric f-low is not supported!")

    twicePNOrder = ethinca_order_from_string(ethincaParams.pnOrder)

    piFl = PI * f0
    totalMass, eta = pnutils.mass1_mass2_to_mtotal_eta(mass1, mass2)
    totalMass = totalMass * MTSUN_SI
    v0cube = totalMass * piFl
    v0 = v0cube**(1. / 3.)

    # Get theoretical cutoff frequency and work out the closest
    # frequency for which moments were calculated
    fMax_theor = pnutils.frequency_cutoff_from_name(ethincaParams.cutoff,
                                                    mass1, mass2, spin1z,
                                                    spin2z)
    fMaxes = metricParams.moments['J4'].keys()
    fMaxIdx = abs(numpy.array(fMaxes, dtype=float) - fMax_theor).argmin()
    fMax = fMaxes[fMaxIdx]

    # Set the appropriate moments
    Js = numpy.zeros([18, 3], dtype=float)
    for i in range(18):
        Js[i, 0] = metricParams.moments['J%d' % (i)][fMax]
        Js[i, 1] = metricParams.moments['log%d' % (i)][fMax]
        Js[i, 2] = metricParams.moments['loglog%d' % (i)][fMax]

    # Compute the time-dependent metric term.
    two_pi_flower_sq = TWOPI * f0 * TWOPI * f0
    gammaVals = numpy.zeros([6], dtype=float)
    gammaVals[0] = 0.5 * two_pi_flower_sq * \
                    ( Js[(1,0)] - (Js[(4,0)]*Js[(4,0)]) )

    # If mass terms not required stop here
    if not full_ethinca:
        return fMax_theor, gammaVals

    # 3pN is a mess, so split it into pieces
    a0 = 11583231236531 / 200286535680 - 5 * PI * PI - 107 * GAMMA / 14
    a1 = (-15737765635 / 130056192 + 2255 * PI * PI / 512) * eta
    a2 = (76055 / 73728) * eta * eta
    a3 = (-127825 / 55296) * eta * eta * eta
    alog = numpy.log(4 * v0)  # Log terms are tricky - be careful

    # Get the Psi coefficients
    Psi = [{}, {}]  #Psi = numpy.zeros([2,8,2],dtype=float)
    Psi[0][0, 0] = 3 / 5
    Psi[0][2, 0] = (743 / 756 + 11 * eta / 3) * v0 * v0
    Psi[0][3, 0] = 0.
    Psi[0][4,0] = (-3058673/508032 + 5429*eta/504 + 617*eta*eta/24)\
                    *v0cube*v0
    Psi[0][5, 1] = (-7729 * PI / 126) * v0cube * v0 * v0 / 3
    Psi[0][6,0] = (128/15)*(-3*a0 - a1 + a2 + 3*a3 + 107*(1+3*alog)/14)\
                    *v0cube*v0cube
    Psi[0][6, 1] = (6848 / 35) * v0cube * v0cube / 3
    Psi[0][7, 0] = (-15419335 / 63504 -
                    75703 * eta / 756) * PI * v0cube * v0cube * v0

    Psi[1][0, 0] = 0.
    Psi[1][2, 0] = (3715 / 12096 - 55 * eta / 96) / PI / v0
    Psi[1][3, 0] = -3 / 2
    Psi[1][4,0] = (15293365/4064256 - 27145*eta/16128 - 3085*eta*eta/384)\
                    *v0/PI
    Psi[1][5, 1] = (193225 / 8064) * v0 * v0 / 3
    Psi[1][6,0] = (4/PI)*(2*a0 + a1/3 - 4*a2/3 - 3*a3 -107*(1+6*alog)/42)\
                    *v0cube
    Psi[1][6, 1] = (-428 / PI / 7) * v0cube / 3
    Psi[1][7,0] = (77096675/1161216 + 378515*eta/24192 + 74045*eta*eta/8064)\
                    *v0cube*v0

    # Set the appropriate moments
    Js = numpy.zeros([18, 3], dtype=float)
    for i in range(18):
        Js[i, 0] = metricParams.moments['J%d' % (i)][fMax]
        Js[i, 1] = metricParams.moments['log%d' % (i)][fMax]
        Js[i, 2] = metricParams.moments['loglog%d' % (i)][fMax]

    # Calculate the g matrix
    PNterms = [(0, 0), (2, 0), (3, 0), (4, 0), (5, 1), (6, 0), (6, 1), (7, 0)]
    PNterms = [term for term in PNterms if term[0] <= twicePNOrder]

    # Now can compute the mass-dependent gamma values
    for m in [0, 1]:
        for k in PNterms:
            gammaVals[1+m] += 0.5 * two_pi_flower_sq * Psi[m][k] * \
                                ( Js[(9-k[0],k[1])]
                                - Js[(12-k[0],k[1])] * Js[(4,0)] )

    g = numpy.zeros([2, 2], dtype=float)
    for (m, n) in [(0, 0), (0, 1), (1, 1)]:
        for k in PNterms:
            for l in PNterms:
                g[m,n] += Psi[m][k] * Psi[n][l] * \
                        ( Js[(17-k[0]-l[0], k[1]+l[1])]
                        - Js[(12-k[0],k[1])] * Js[(12-l[0],l[1])] )
        g[m, n] = 0.5 * two_pi_flower_sq * g[m, n]
        g[n, m] = g[m, n]

    gammaVals[3] = g[0, 0]
    gammaVals[4] = g[0, 1]
    gammaVals[5] = g[1, 1]

    return fMax_theor, gammaVals
示例#6
0
def output_sngl_inspiral_table(outputFile, tempBank, metricParams,
                               ethincaParams, programName="", optDict = None,
                               outdoc=None, **kwargs):
    """
    Function that converts the information produced by the various pyCBC bank
    generation codes into a valid LIGOLW xml file containing a sngl_inspiral
    table and outputs to file.

    Parameters
    -----------
    outputFile : string
        Name of the file that the bank will be written to
    tempBank : iterable
        Each entry in the tempBank iterable should be a sequence of
        [mass1,mass2,spin1z,spin2z] in that order.
    metricParams : metricParameters instance
        Structure holding all the options for construction of the metric
        and the eigenvalues, eigenvectors and covariance matrix
        needed to manipulate the space.
    ethincaParams: {ethincaParameters instance, None}
        Structure holding options relevant to the ethinca metric computation
        including the upper frequency cutoff to be used for filtering.
        NOTE: The computation is currently only valid for non-spinning systems
        and uses the TaylorF2 approximant.
    programName (key-word-argument) : string
        Name of the executable that has been run
    optDict (key-word argument) : dictionary
        Dictionary of the command line arguments passed to the program
    outdoc (key-word argument) : ligolw xml document
        If given add template bank to this representation of a xml document and
        write to disk. If not given create a new document.
    kwargs : key-word arguments
        All other key word arguments will be passed directly to
        ligolw_process.register_to_xmldoc
    """
    if optDict is None:
        optDict = {}
    if outdoc is None:
        outdoc = ligolw.Document()
        outdoc.appendChild(ligolw.LIGO_LW())

    # get IFO to put in search summary table
    ifos = []
    if 'channel_name' in optDict.keys():
        if optDict['channel_name'] is not None:
            ifos = [optDict['channel_name'][0:2]]

    proc_id = ligolw_process.register_to_xmldoc(outdoc, programName, optDict,
                                                ifos=ifos, **kwargs).process_id
    sngl_inspiral_table = convert_to_sngl_inspiral_table(tempBank, proc_id)
    # Calculate Gamma components if needed
    if ethincaParams is not None:
        if ethincaParams.doEthinca:
            for sngl in sngl_inspiral_table:
                # Set tau_0 and tau_3 values needed for the calculation of
                # ethinca metric distances
                (sngl.tau0,sngl.tau3) = pnutils.mass1_mass2_to_tau0_tau3(
                    sngl.mass1, sngl.mass2, metricParams.f0)
                fMax_theor, GammaVals = calculate_ethinca_metric_comps(
                    metricParams, ethincaParams,
                    sngl.mass1, sngl.mass2, spin1z=sngl.spin1z,
                    spin2z=sngl.spin2z, full_ethinca=ethincaParams.full_ethinca)
                # assign the upper frequency cutoff and Gamma0-5 values
                sngl.f_final = fMax_theor
                for i in xrange(len(GammaVals)):
                    setattr(sngl, "Gamma"+str(i), GammaVals[i])
        # If Gamma metric components are not wanted, assign f_final from an
        # upper frequency cutoff specified in ethincaParams
        elif ethincaParams.cutoff is not None:
            for sngl in sngl_inspiral_table:
                sngl.f_final = pnutils.frequency_cutoff_from_name(
                    ethincaParams.cutoff,
                    sngl.mass1, sngl.mass2, sngl.spin1z, sngl.spin2z)

    # set per-template low-frequency cutoff
    if 'f_low_column' in optDict and 'f_low' in optDict and \
            optDict['f_low_column'] is not None:
        for sngl in sngl_inspiral_table:
            setattr(sngl, optDict['f_low_column'], optDict['f_low'])

    outdoc.childNodes[0].appendChild(sngl_inspiral_table)

    # get times to put in search summary table
    start_time = 0
    end_time = 0
    if 'gps_start_time' in optDict.keys() and 'gps_end_time' in optDict.keys():
        start_time = optDict['gps_start_time']
        end_time = optDict['gps_end_time']

    # make search summary table
    search_summary_table = lsctables.New(lsctables.SearchSummaryTable)
    search_summary = return_search_summary(start_time, end_time,
                               len(sngl_inspiral_table), ifos, **kwargs)
    search_summary_table.append(search_summary)
    outdoc.childNodes[0].appendChild(search_summary_table)

    # write the xml doc to disk
    ligolw_utils.write_filename(outdoc, outputFile,
                                gz=outputFile.endswith('.gz'))
示例#7
0
def calculate_ethinca_metric_comps(metricParams, ethincaParams, mass1, mass2,
                                   spin1z=0., spin2z=0., full_ethinca=True):
    """
    Calculate the Gamma components needed to use the ethinca metric.
    At present this outputs the standard TaylorF2 metric over the end time
    and chirp times \tau_0 and \tau_3.
    A desirable upgrade might be to use the \chi coordinates [defined WHERE?]
    for metric distance instead of \tau_0 and \tau_3.
    The lower frequency cutoff is currently hard-coded to be the same as the
    bank layout options fLow and f0 (which must be the same as each other).

    Parameters
    -----------
    metricParams : metricParameters instance
        Structure holding all the options for construction of the metric
        and the eigenvalues, eigenvectors and covariance matrix
        needed to manipulate the space.
    ethincaParams : ethincaParameters instance
        Structure holding options relevant to the ethinca metric computation.
    mass1 : float
        Mass of the heavier body in the considered template.
    mass2 : float
        Mass of the lighter body in the considered template.
    spin1z : float (optional, default=0)
        Spin of the heavier body in the considered template.
    spin2z : float (optional, default=0)
        Spin of the lighter body in the considered template.
    full_ethinca : boolean (optional, default=True)
        If True calculate the ethinca components in all 3 directions (mass1,
        mass2 and time). If False calculate only the time component (which is
        stored in Gamma0).
    Returns
    --------
    fMax_theor : float
        Value of the upper frequency cutoff given by the template parameters
        and the cutoff formula requested.

    gammaVals : numpy_array
        Array holding 6 independent metric components in
        (end_time, tau_0, tau_3) coordinates to be stored in the Gamma0-5
        slots of a SnglInspiral object.
    """
    if (float(spin1z) != 0. or float(spin2z) != 0.) and full_ethinca:
        raise NotImplementedError("Ethinca cannot at present be calculated "
                                  "for nonzero component spins!")
    f0 = metricParams.f0
    if f0 != metricParams.fLow:
        raise ValueError("If calculating ethinca the bank f0 value must be "
                         "equal to f-low!")
    if ethincaParams.fLow is not None and (
        ethincaParams.fLow != metricParams.fLow):
        raise NotImplementedError("An ethinca metric f-low different from the"
                                  " bank metric f-low is not supported!")

    twicePNOrder = ethinca_order_from_string(ethincaParams.pnOrder)

    piFl = PI * f0
    totalMass, eta = pnutils.mass1_mass2_to_mtotal_eta(mass1, mass2)
    totalMass = totalMass * MTSUN_SI
    v0cube = totalMass*piFl
    v0 = v0cube**(1./3.)

    # Get theoretical cutoff frequency and work out the closest
    # frequency for which moments were calculated
    fMax_theor = pnutils.frequency_cutoff_from_name(
        ethincaParams.cutoff, mass1, mass2, spin1z, spin2z)
    fMaxes = metricParams.moments['J4'].keys()
    fMaxIdx = abs(numpy.array(fMaxes,dtype=float) - fMax_theor).argmin()
    fMax = fMaxes[fMaxIdx]

    # Set the appropriate moments
    Js = numpy.zeros([18,3],dtype=float)
    for i in range(18):
        Js[i,0] = metricParams.moments['J%d'%(i)][fMax]
        Js[i,1] = metricParams.moments['log%d'%(i)][fMax]
        Js[i,2] = metricParams.moments['loglog%d'%(i)][fMax]

    # Compute the time-dependent metric term.
    two_pi_flower_sq = TWOPI * f0 * TWOPI * f0
    gammaVals = numpy.zeros([6],dtype=float)
    gammaVals[0] = 0.5 * two_pi_flower_sq * \
                    ( Js[(1,0)] - (Js[(4,0)]*Js[(4,0)]) )

    # If mass terms not required stop here
    if not full_ethinca:
        return fMax_theor, gammaVals

    # 3pN is a mess, so split it into pieces
    a0 = 11583231236531/200286535680 - 5*PI*PI - 107*GAMMA/14
    a1 = (-15737765635/130056192 + 2255*PI*PI/512)*eta
    a2 = (76055/73728)*eta*eta
    a3 = (-127825/55296)*eta*eta*eta
    alog = numpy.log(4*v0) # Log terms are tricky - be careful

    # Get the Psi coefficients
    Psi = [{},{}] #Psi = numpy.zeros([2,8,2],dtype=float)
    Psi[0][0,0] = 3/5
    Psi[0][2,0] = (743/756 + 11*eta/3)*v0*v0
    Psi[0][3,0] = 0.
    Psi[0][4,0] = (-3058673/508032 + 5429*eta/504 + 617*eta*eta/24)\
                    *v0cube*v0
    Psi[0][5,1] = (-7729*PI/126)*v0cube*v0*v0/3
    Psi[0][6,0] = (128/15)*(-3*a0 - a1 + a2 + 3*a3 + 107*(1+3*alog)/14)\
                    *v0cube*v0cube
    Psi[0][6,1] = (6848/35)*v0cube*v0cube/3
    Psi[0][7,0] = (-15419335/63504 - 75703*eta/756)*PI*v0cube*v0cube*v0

    Psi[1][0,0] = 0.
    Psi[1][2,0] = (3715/12096 - 55*eta/96)/PI/v0;
    Psi[1][3,0] = -3/2
    Psi[1][4,0] = (15293365/4064256 - 27145*eta/16128 - 3085*eta*eta/384)\
                    *v0/PI
    Psi[1][5,1] = (193225/8064)*v0*v0/3
    Psi[1][6,0] = (4/PI)*(2*a0 + a1/3 - 4*a2/3 - 3*a3 -107*(1+6*alog)/42)\
                    *v0cube
    Psi[1][6,1] = (-428/PI/7)*v0cube/3
    Psi[1][7,0] = (77096675/1161216 + 378515*eta/24192 + 74045*eta*eta/8064)\
                    *v0cube*v0

    # Set the appropriate moments
    Js = numpy.zeros([18,3],dtype=float)
    for i in range(18):
        Js[i,0] = metricParams.moments['J%d'%(i)][fMax]
        Js[i,1] = metricParams.moments['log%d'%(i)][fMax]
        Js[i,2] = metricParams.moments['loglog%d'%(i)][fMax]

    # Calculate the g matrix
    PNterms = [(0,0),(2,0),(3,0),(4,0),(5,1),(6,0),(6,1),(7,0)]
    PNterms = [term for term in PNterms if term[0] <= twicePNOrder]

    # Now can compute the mass-dependent gamma values
    for m in [0, 1]:
        for k in PNterms:
            gammaVals[1+m] += 0.5 * two_pi_flower_sq * Psi[m][k] * \
                                ( Js[(9-k[0],k[1])]
                                - Js[(12-k[0],k[1])] * Js[(4,0)] )

    g = numpy.zeros([2,2],dtype=float)
    for (m,n) in [(0,0),(0,1),(1,1)]:
        for k in PNterms:
            for l in PNterms:
                g[m,n] += Psi[m][k] * Psi[n][l] * \
                        ( Js[(17-k[0]-l[0], k[1]+l[1])]
                        - Js[(12-k[0],k[1])] * Js[(12-l[0],l[1])] )
        g[m,n] = 0.5 * two_pi_flower_sq * g[m,n]
        g[n,m] = g[m,n]

    gammaVals[3] = g[0,0]
    gammaVals[4] = g[0,1]
    gammaVals[5] = g[1,1]

    return fMax_theor, gammaVals