#include <lal/LALDatatypes.h>Include dependency graph for LALSimInspiral.h:

Go to the source code of this file.
Defines | |
| #define | LAL_PN_MODE_L_MAX 3 |
Functions | |
| NRCSID (LALSIMINSPIRALH,"$Id: LALSimInspiral.h,v 1.4 2008/03/20 00:31:57 jolien Exp $") | |
| COMPLEX16 | XLALSimInspiralPNMode22 (REAL8 x, REAL8 phi, REAL8 logx, REAL8 m1, REAL8 m2, REAL8 r, int O) |
| Computes h(2,2) mode of spherical harmonic decomposition of the post-Newtonian inspiral waveform. | |
| COMPLEX16 | XLALSimInspiralPNMode21 (REAL8 x, REAL8 phi, REAL8 logx, REAL8 m1, REAL8 m2, REAL8 r, int O) |
| Computes h(2,1) mode of spherical harmonic decomposition of the post-Newtonian inspiral waveform. | |
| COMPLEX16 | XLALSimInspiralPNMode33 (REAL8 x, REAL8 phi, REAL8 logx, REAL8 m1, REAL8 m2, REAL8 r, int O) |
| Computes h(3,3) mode of spherical harmonic decomposition of the post-Newtonian inspiral waveform. | |
| COMPLEX16 | XLALSimInspiralPNMode32 (REAL8 x, REAL8 phi, REAL8 logx, REAL8 m1, REAL8 m2, REAL8 r, int O) |
| Computes h(3,2) mode of spherical harmonic decomposition of the post-Newtonian inspiral waveform. | |
| COMPLEX16 | XLALSimInspiralPNMode31 (REAL8 x, REAL8 phi, REAL8 logx, REAL8 m1, REAL8 m2, REAL8 r, int O) |
| Computes h(3,1) mode of spherical harmonic decomposition of the post-Newtonian inspiral waveform. | |
| COMPLEX16 | XLALSpinWeightedSphericalHarmonic (REAL8 theta, REAL8 phi, int s, int l, int m) |
| Computes the (s)Y(l,m) spin-weighted spherical harmonic. | |
| int | XLALSimAddMode (REAL8TimeSeries *hplus, REAL8TimeSeries *hcross, COMPLEX16TimeSeries *hmode, REAL8 theta, REAL8 phi, int l, int m, int sym) |
| Multiplies a mode h(l,m) by a spin-2 weighted spherical harmonic to obtain hplus - i hcross, which is added to the time series. | |
| REAL8 | XLALSimInspiralPNAngularAcceleration (REAL8 x, REAL8 m1, REAL8 m2, int O) |
| Computes the rate of increase of the orbital frequency for a post-Newtonian inspiral. | |
| REAL8 | XLALSimInspiralPNAngularVelocity (REAL8 x, REAL8 m1, REAL8 m2) |
| Computes the orbital angular velocity from the quantity x. | |
| REAL8 | XLALSimInspiralPNEnergy (REAL8 x, REAL8 m1, REAL8 m2, int O) |
| Computes the orbital energy at a fixed frequency and pN order. | |
| int | XLALSimInspiralPNEvolveOrbitTaylorT4 (REAL8TimeSeries **x, REAL8TimeSeries **phi, LIGOTimeGPS *tc, REAL8 phic, REAL8 deltaT, REAL8 m1, REAL8 m2, REAL8 fmin, int O) |
| Evolves a post-Newtonian orbit using the Taylor T4 method. | |
| COMPLEX16TimeSeries * | XLALCreateSimInspiralPNModeCOMPLEX16TimeSeries (REAL8TimeSeries *x, REAL8TimeSeries *phi, REAL8 x0, REAL8 m1, REAL8 m2, REAL8 r, int O, int l, int m) |
| Computes h(l,m) mode timeseries of spherical harmonic decomposition of the post-Newtonian inspiral waveform. | |
| int | XLALSimInspiralPNPolarizationWaveforms (REAL8TimeSeries **hplus, REAL8TimeSeries **hcross, REAL8TimeSeries *x, REAL8TimeSeries *phi, REAL8 x0, REAL8 m1, REAL8 m2, REAL8 r, REAL8 i, int O) |
| Given an orbit evolution phasing, construct the waveform h+ and hx. | |
| int | XLALSimInspiralPN (REAL8TimeSeries **hplus, REAL8TimeSeries **hcross, LIGOTimeGPS *tc, REAL8 phic, REAL8 deltaT, REAL8 m1, REAL8 m2, REAL8 fmin, REAL8 r, REAL8 i, int O) |
| Driver routine to compute the post-Newtonian inspiral waveform. | |
| int | XLALSimInspiralPNRestricted (REAL8TimeSeries **hplus, REAL8TimeSeries **hcross, LIGOTimeGPS *tc, REAL8 phic, REAL8 deltaT, REAL8 m1, REAL8 m2, REAL8 fmin, REAL8 r, REAL8 i, int O) |
| Driver routine to compute the restricted post-Newtonian inspiral waveform. | |
| #define LAL_PN_MODE_L_MAX 3 |
Definition at line 22 of file LALSimInspiral.h.
| NRCSID | ( | LALSIMINSPIRALH | , | |
| "$Id: LALSimInspiral. | h, | |||
| v 1.4 2008/03/20 00:31:57 jolien Exp $" | ||||
| ) |
| COMPLEX16 XLALSimInspiralPNMode22 | ( | REAL8 | x, | |
| REAL8 | phi, | |||
| REAL8 | logx, | |||
| REAL8 | m1, | |||
| REAL8 | m2, | |||
| REAL8 | r, | |||
| int | O | |||
| ) |
Computes h(2,2) mode of spherical harmonic decomposition of the post-Newtonian inspiral waveform.
Implements Equation (79) of: Lawrence E. Kidder, "Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit", Physical Review D 77, 044016 (2008), arXiv:0710.0614v1 [gr-qc].
| x | post-Newtonian parameter |
| phi | orbital phase |
| logx | log(x/x0) tail gauge parameter |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| r | distance of source |
| O | twice post-Newtonian order |
Definition at line 38 of file LALSimInspiralPNMode.c.
| COMPLEX16 XLALSimInspiralPNMode21 | ( | REAL8 | x, | |
| REAL8 | phi, | |||
| REAL8 | logx, | |||
| REAL8 | m1, | |||
| REAL8 | m2, | |||
| REAL8 | r, | |||
| int | O | |||
| ) |
Computes h(2,1) mode of spherical harmonic decomposition of the post-Newtonian inspiral waveform.
Implements Equation (80) of: Lawrence E. Kidder, "Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit", Physical Review D 77, 044016 (2008), arXiv:0710.0614v1 [gr-qc].
| x | post-Newtonian parameter |
| phi | orbital phase |
| logx | log(x/x0) tail gauge parameter |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| r | distance of source |
| O | twice post-Newtonian order |
Definition at line 92 of file LALSimInspiralPNMode.c.
| COMPLEX16 XLALSimInspiralPNMode33 | ( | REAL8 | x, | |
| REAL8 | phi, | |||
| REAL8 | logx, | |||
| REAL8 | m1, | |||
| REAL8 | m2, | |||
| REAL8 | r, | |||
| int | O | |||
| ) |
Computes h(3,3) mode of spherical harmonic decomposition of the post-Newtonian inspiral waveform.
Implements Equation (82) of: Lawrence E. Kidder, "Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit", Physical Review D 77, 044016 (2008), arXiv:0710.0614v1 [gr-qc].
| x | post-Newtonian parameter |
| phi | orbital phase |
| logx | log(x/x0) tail gauge parameter |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| r | distance of source |
| O | twice post-Newtonian order |
Definition at line 143 of file LALSimInspiralPNMode.c.
| COMPLEX16 XLALSimInspiralPNMode32 | ( | REAL8 | x, | |
| REAL8 | phi, | |||
| REAL8 | logx, | |||
| REAL8 | m1, | |||
| REAL8 | m2, | |||
| REAL8 | r, | |||
| int | O | |||
| ) |
Computes h(3,2) mode of spherical harmonic decomposition of the post-Newtonian inspiral waveform.
Implements Equation (83) of: Lawrence E. Kidder, "Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit", Physical Review D 77, 044016 (2008), arXiv:0710.0614v1 [gr-qc].
| x | post-Newtonian parameter |
| phi | orbital phase |
| logx | log(x/x0) tail gauge parameter |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| r | distance of source |
| O | twice post-Newtonian order |
Definition at line 195 of file LALSimInspiralPNMode.c.
| COMPLEX16 XLALSimInspiralPNMode31 | ( | REAL8 | x, | |
| REAL8 | phi, | |||
| REAL8 | logx, | |||
| REAL8 | m1, | |||
| REAL8 | m2, | |||
| REAL8 | r, | |||
| int | O | |||
| ) |
Computes h(3,1) mode of spherical harmonic decomposition of the post-Newtonian inspiral waveform.
Implements Equation (84) of: Lawrence E. Kidder, "Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit", Physical Review D 77, 044016 (2008), arXiv:0710.0614v1 [gr-qc].
| x | post-Newtonian parameter |
| phi | orbital phase |
| logx | log(x/x0) tail gauge parameter |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| r | distance of source |
| O | twice post-Newtonian order |
Definition at line 244 of file LALSimInspiralPNMode.c.
Computes the (s)Y(l,m) spin-weighted spherical harmonic.
From somewhere ....
See also: Implements Equations (II.9)-(II.13) of D. A. Brown, S. Fairhurst, B. Krishnan, R. A. Mercer, R. K. Kopparapu, L. Santamaria, and J. T. Whelan, "Data formats for numerical relativity waves", arXiv:0709.0093v1 (2007).
Currently only supports s=-2, l=2,3,4,5 modes.
| theta | polar angle (rad) |
| phi | azimuthal angle (rad) |
| s | spin weight |
| l | mode number l |
| m | mode number m |
Definition at line 53 of file LALSimInspiral.c.
| int XLALSimAddMode | ( | REAL8TimeSeries * | hplus, | |
| REAL8TimeSeries * | hcross, | |||
| COMPLEX16TimeSeries * | hmode, | |||
| REAL8 | theta, | |||
| REAL8 | phi, | |||
| int | l, | |||
| int | m, | |||
| int | sym | |||
| ) |
Multiplies a mode h(l,m) by a spin-2 weighted spherical harmonic to obtain hplus - i hcross, which is added to the time series.
Implements the sum of a single term of Eq. (11) of: Lawrence E. Kidder, "Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit", Physical Review D 77, 044016 (2008), arXiv:0710.0614v1 [gr-qc].
If sym is non-zero, symmetrically add the m and -m terms assuming that h(l,-m) = (-1)^l h(l,m)*; see Eq. (78) ibid.
| hplus | +-polarization waveform |
| hcross | x-polarization waveform |
| hmode | complex mode h(l,m) |
| theta | polar angle (rad) |
| phi | azimuthal angle (rad) |
| l | mode number l |
| m | mode number m |
| sym | flag to add -m mode too |
Definition at line 240 of file LALSimInspiral.c.
Computes the rate of increase of the orbital frequency for a post-Newtonian inspiral.
This function returns dx/dt rather than the true angular acceleration.
Implements Equation (6) of Yi Pan, Alessandra Buonanno, Yanbei Chen, and Michele Vallisneri, "A physical template family for gravitational waves from precessing binaries of spinning compact objects: Application to single-spin binaries" arXiv:gr-qc/0310034v3 (2007).
Note: this equation is actually dx/dt rather than (domega/dt)/(omega)^2 so the leading coefficient is different. Also, this function applies for non-spinning objects.
Compare the overall coefficient, with nu=1/4, to Equation (45) of Michael Boyle, Duncan A. Brown, Lawrence E. Kidder, Abdul H. Mroue, Harald P. Pfeiffer, Mark A. Scheel, Gregory B. Cook, and Saul A. Teukolsky "High-accuracy comparison of numerical relativity simulations with post-Newtonian expansions" arXiv:0710.0158v1 (2007).
| x | post-Newtonian parameter |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| O | twice post-Newtonian order |
Definition at line 305 of file LALSimInspiral.c.
Computes the orbital angular velocity from the quantity x.
This is from the definition of x.
Implements Equation (46) of Michael Boyle, Duncan A. Brown, Lawrence E. Kidder, Abdul H. Mroue, Harald P. Pfeiffer, Mark A. Scheel, Gregory B. Cook, and Saul A. Teukolsky "High-accuracy comparison of numerical relativity simulations with post-Newtonian expansions" arXiv:0710.0158v1 (2007).
| x | post-Newtonian parameter |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
Definition at line 356 of file LALSimInspiral.c.
Computes the orbital energy at a fixed frequency and pN order.
Implements Equation (152) of Luc Blanchet, "Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries", http://www.livingreviews.org/lrr-2006-4/index.html
This is the same as Equation (10) (where the spin of the objects is zero) of: Yi Pan, Alessandra Buonanno, Yanbei Chen, and Michele Vallisneri, "A physical template family for gravitational waves from precessing binaries of spinning compact objects: Application to single-spin binaries" arXiv:gr-qc/0310034v3 (2007). Note: this equation is actually dx/dt rather than (domega/dt)/(omega)^2 so the leading coefficient is different.
| x | post-Newtonian parameter |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| O | twice post-Newtonian order |
Definition at line 387 of file LALSimInspiral.c.
| int XLALSimInspiralPNEvolveOrbitTaylorT4 | ( | REAL8TimeSeries ** | x, | |
| REAL8TimeSeries ** | phi, | |||
| LIGOTimeGPS * | tc, | |||
| REAL8 | phic, | |||
| REAL8 | deltaT, | |||
| REAL8 | m1, | |||
| REAL8 | m2, | |||
| REAL8 | fmin, | |||
| int | O | |||
| ) |
Evolves a post-Newtonian orbit using the Taylor T4 method.
See: Michael Boyle, Duncan A. Brown, Lawrence E. Kidder, Abdul H. Mroue, Harald P. Pfeiffer, Mark A. Scheel, Gregory B. Cook, and Saul A. Teukolsky "High-accuracy comparison of numerical relativity simulations with post-Newtonian expansions" arXiv:0710.0158v1 (2007).
| x | post-Newtonian parameter [returned] |
| phi | orbital phase [returned] |
| tc | coalescence time |
| phic | coalescence phase |
| deltaT | sampling interval |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| fmin | start frequency |
| O | twice post-Newtonian order |
Definition at line 445 of file LALSimInspiral.c.
| COMPLEX16TimeSeries* XLALCreateSimInspiralPNModeCOMPLEX16TimeSeries | ( | REAL8TimeSeries * | x, | |
| REAL8TimeSeries * | phi, | |||
| REAL8 | x0, | |||
| REAL8 | m1, | |||
| REAL8 | m2, | |||
| REAL8 | r, | |||
| int | O, | |||
| int | l, | |||
| int | m | |||
| ) |
Computes h(l,m) mode timeseries of spherical harmonic decomposition of the post-Newtonian inspiral waveform.
See Eqns. (79)-(116) of: Lawrence E. Kidder, "Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit", Physical Review D 77, 044016 (2008), arXiv:0710.0614v1 [gr-qc].
| x | post-Newtonian parameter |
| phi | orbital phase |
| x0 | tail-term gauge choice thing (if you don't know, just set it to zero) |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| r | distance of source |
| O | twice post-Newtonain order |
| l | mode number l |
| m | mode number m |
Definition at line 550 of file LALSimInspiral.c.
| int XLALSimInspiralPNPolarizationWaveforms | ( | REAL8TimeSeries ** | hplus, | |
| REAL8TimeSeries ** | hcross, | |||
| REAL8TimeSeries * | x, | |||
| REAL8TimeSeries * | phi, | |||
| REAL8 | x0, | |||
| REAL8 | m1, | |||
| REAL8 | m2, | |||
| REAL8 | r, | |||
| REAL8 | i, | |||
| int | O | |||
| ) |
Given an orbit evolution phasing, construct the waveform h+ and hx.
Implements Equation (11) of: Lawrence E. Kidder, "Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit", Physical Review D 77, 044016 (2008), arXiv:0710.0614v1 [gr-qc].
| hplus | +-polarization waveform [returned] |
| hcross | x-polarization waveform [returned] |
| x | post-Newtonian parameter |
| phi | orbital phase |
| x0 | tail-term gauge choice thing (if you don't know, just set it to zero) |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| r | distance of source |
| i | inclination of source (rad) |
| O | twice post-Newtonian order |
Definition at line 608 of file LALSimInspiral.c.
| int XLALSimInspiralPN | ( | REAL8TimeSeries ** | hplus, | |
| REAL8TimeSeries ** | hcross, | |||
| LIGOTimeGPS * | tc, | |||
| REAL8 | phic, | |||
| REAL8 | deltaT, | |||
| REAL8 | m1, | |||
| REAL8 | m2, | |||
| REAL8 | fmin, | |||
| REAL8 | r, | |||
| REAL8 | i, | |||
| int | O | |||
| ) |
Driver routine to compute the post-Newtonian inspiral waveform.
This routine uses the same pN order for phasing and amplitude (unless the order is -1 in which case the highest available order is used for both of these -- which might not be the same).
Log terms in amplitudes are ignored. This is a gauge choice.
| hplus | +-polarization waveform |
| hcross | x-polarization waveform |
| tc | coalescence time |
| phic | coalescence phase |
| deltaT | sampling interval |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| fmin | start frequency |
| r | distance of source |
| i | inclination of source (rad) |
| O | twice post-Newtonian order |
Definition at line 693 of file LALSimInspiral.c.
| int XLALSimInspiralPNRestricted | ( | REAL8TimeSeries ** | hplus, | |
| REAL8TimeSeries ** | hcross, | |||
| LIGOTimeGPS * | tc, | |||
| REAL8 | phic, | |||
| REAL8 | deltaT, | |||
| REAL8 | m1, | |||
| REAL8 | m2, | |||
| REAL8 | fmin, | |||
| REAL8 | r, | |||
| REAL8 | i, | |||
| int | O | |||
| ) |
Driver routine to compute the restricted post-Newtonian inspiral waveform.
This routine computes the phasing to the specified order, but only computes the amplitudes to the Newtonian (quadrupole) order.
Log terms in amplitudes are ignored. This is a gauge choice.
| hplus | +-polarization waveform |
| hcross | x-polarization waveform |
| tc | coalescence time |
| phic | coalescence phase |
| deltaT | sampling interval |
| m1 | mass of companion 1 |
| m2 | mass of companion 2 |
| fmin | start frequency |
| r | distance of source |
| i | inclination of source (rad) |
| O | twice post-Newtonian phase order |
Definition at line 719 of file LALSimInspiral.c.
1.5.2