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Source-Frame and Detector-Frame Parameters

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A compact-binary waveform is generated in a local source frame but recorded after propagation through an expanding universe. Cosmological expansion stretches every source-frame time and wavelength by the same factor 1+z1+z. Consequently, detectors measure redshifted dimensional masses and frequencies, while mass ratios, dimensionless spins, and geometric angles are unchanged. Distance is subtler: the strain amplitude contains the luminosity distance DLD_L, but converting DLD_L into zz requires a cosmological model or external information.

Helpful background. Einstein Equations supplies local source dynamics and cosmological geometry; Waves, Green Functions, and Geometric Optics supplies phase and amplitude transport; Relativistic Two-Body Dynamics supplies the intrinsic binary parameters; Gravitational Radiation and Waveforms supplies strain modes and flux conventions; and Computational Relativity supplies source-frame strong-field waveforms.

On scales large compared with the source, write a Friedmann–Lemaître–Robertson–Walker metric in conformal time η\eta as

ds2=a2(η)[−dη2+dχ2+SK2(χ)dΩ2],ds^2=a^2(\eta) \left[-d\eta^2+d\chi^2+S_K^2(\chi)d\Omega^2\right],

where SK(χ)S_K(\chi) encodes the spatial curvature. A radial geometric-optics ray obeys dχ=±dηd\chi=\pm d\eta. Its comoving wave number is conserved, whereas a comoving observer measures physical angular frequency ω∝a−1\omega\propto a^{-1}. If the wave is emitted at scale factor aea_{\mathrm e} and detected at a0a_0, then

1+z=a0ae,fdet=fsrc1+z,dtdet=(1+z)dtsrc.1+z=\frac{a_0}{a_{\mathrm e}}, \qquad f_{\rm det}=\frac{f_{\rm src}}{1+z}, \qquad dt_{\rm det}=(1+z)dt_{\rm src}.

The last two relations are the same phase statement: dΦ=2πfsrcdtsrc=2πfdetdtdetd\Phi=2\pi f_{\rm src}dt_{\rm src}=2\pi f_{\rm det}dt_{\rm det}. Cosmological propagation of tensor waves and its redshift scaling are developed in Caprini and Figueroa 2018, §§2–3.

These are source-to-observer relations, not Doppler corrections inside the binary model. A source-frame reference frequency must therefore be divided by 1+z1+z before it is compared with a detector-frame reference frequency.

The usual binary-waveform scaling treats zz as constant during the observation and assumes homogeneous geometric-optics propagation between comoving source and observer frames. Redshift drift, peculiar accelerations, lensing, and observer aberration require additional mappings. In particular, the statement that angles are unchanged concerns cosmological dilation itself; it does not say that lensing or a change of observer velocity cannot change an apparent direction.

Local vacuum binary dynamics have no independent absolute scale. Let MsrcM_{\mathrm{src}} be a source-frame mass scale, λ\lambda any dimensionless intrinsic parameters, and H\mathcal H a dimensionless waveform shape. The observed complex strain can be organized as

h+(tdet)−ih×(tdet)=GMzDLH ⁣(tdet−tcGMz;λ,angles),Mz≡(1+z)Msrc.h_+(t_{\rm det})-ih_\times(t_{\rm det}) =\frac{GM_z}{D_L} \mathcal H\!\left( \frac{t_{\rm det}-t_c}{GM_z}; \lambda,\text{angles} \right), \qquad M_z\equiv(1+z)M_{\mathrm{src}}.

Equivalently, the source constructs H=r(h+−ih×)H=r(h_+-ih_\times) from unit-normalized spin-weight −2-2 modes with the e−iωte^{-i\omega t} convention; cosmological propagation replaces the local distance scaling by DLD_L and the source mass scale by MzM_z. The post-Newtonian source waveform and its mass-frequency scaling are organized explicitly in Blanchet 2024, §§3.4.3–3.4.5, pp. 206–219.

The leading chirp makes the degeneracy transparent. In the source frame,

dfsrcdtsrc=965π8/3(GMsrc)5/3fsrc11/3,\frac{df_{\rm src}}{dt_{\rm src}} =\frac{96}{5}\pi^{8/3} (G\mathcal M_{\mathrm{src}})^{5/3}f_{\rm src}^{11/3},

where M=Mν3/5\mathcal M=M\nu^{3/5} is the chirp mass. Since dfdet/dtdet=(1+z)−2dfsrc/dtsrcdf_{\rm det}/dt_{\rm det}=(1+z)^{-2}df_{\rm src}/dt_{\rm src}, substitution of fsrc=(1+z)fdetf_{\rm src}=(1+z)f_{\rm det} gives

dfdetdtdet=965π8/3(GMz)5/3fdet11/3,Mz=(1+z)Msrc.\frac{df_{\rm det}}{dt_{\rm det}} =\frac{96}{5}\pi^{8/3} (G\mathcal M_z)^{5/3}f_{\rm det}^{11/3}, \qquad \mathcal M_z=(1+z)\mathcal M_{\mathrm{src}}.

Thus an otherwise scale-free gravitational waveform measures Mz\mathcal M_z, not Msrc\mathcal M_{\mathrm{src}} and zz separately. Every dimensional mass transforms in the same way: mA,z=(1+z)mA,srcm_{A,z}=(1+z)m_{A,\rm src}. Ratios such as q=m1/m2q=m_1/m_2 and ν=m1m2/M2\nu=m_1m_2/M^2, and dimensionless spins χA=SA/(GmA2)\boldsymbol\chi_A=\boldsymbol S_A/(Gm_A^2), are invariant.

Luminosity distance and cosmological assumptions

Section titled “Luminosity distance and cosmological assumptions”

Set a0=1a_0=1. In FLRW geometry,

DL(z)=(1+z)SK[χ(z)],χ(z)=∫0zdz′H(z′).D_L(z)=(1+z)S_K[\chi(z)], \qquad \chi(z)=\int_0^z\frac{dz'}{H(z')}.

This formula already shows the division of responsibilities. Wave propagation identifies DLD_L as the amplitude distance. Turning a measured DLD_L into a redshift requires a choice of H(z)H(z) and spatial curvature. The standard relations among comoving, angular-diameter, and luminosity distances, including DL=(1+z)2DAD_L=(1+z)^2D_A, are summarized in Hogg 1999, §§2–7.

Even after choosing a background cosmology, line-of-sight structure perturbs the simple map. For one resolved geometric-optics image, a positive absolute magnification ∣μlens∣\lvert\mu_{\rm lens}\rvert rescales the amplitude as if DLD_L were DL/∣μlens∣D_L/\sqrt{\lvert\mu_{\rm lens}\rvert}. Its arrival-time and Morse-phase shifts must be included separately. Unresolved images or wave-optics diffraction can produce frequency-dependent interference, so they cannot in general be absorbed into one distance. See Gravitational Lensing for that transfer function. Peculiar velocities alter the relation between cosmological redshift and an observed host redshift, especially nearby. These are propagation or environment effects, not changes to the source’s mass ratio or spin.

Redshift is a dilation, not a rotation. Sky direction, binary inclination, polarization angle, orbital phase, precession angles, and dimensionless eccentricity do not acquire factors of 1+z1+z. Their numerical definitions still require declared frames:

  • source modes are referred to a source inertial or coprecessing triad;
  • the line of sight rotates those modes into a transverse polarization basis;
  • detector antenna patterns project that basis onto an instrument.

The mode rotation and cosmological dilation commute because they act on different structures. However, a dimensionless parameter quoted at a reference frequency inherits a frame label indirectly. For example, eccentricity at 20 Hz20\,\mathrm{Hz} detector-frame refers to the source when its frequency was 20(1+z) Hz20(1+z)\,\mathrm{Hz}, so it is not interchangeable with eccentricity at 20 Hz20\,\mathrm{Hz} source-frame.

The mapping can be kept compact:

QuantityDetector/source relationCosmology needed?
Dimensional massmz=(1+z)msrcm_z=(1+z)m_{\rm src}zz needed to recover msrcm_{\rm src}
Frequencyfdet=fsrc/(1+z)f_{\rm det}=f_{\rm src}/(1+z)zz needed for source frequency
Time intervalΔtdet=(1+z)Δtsrc\Delta t_{\rm det}=(1+z)\Delta t_{\rm src}zz needed for source time
Mass ratio, ν\nu, dimensionless spinunchangedno
Angles and dimensionless eccentricityunchanged at corresponding eventsno, but reference frequency must be mapped
Amplitude distancewaveform contains DLD_Lyes, to infer zz from DLD_L

Consistency checks and interpretive limits

Section titled “Consistency checks and interpretive limits”

Three checks catch most frame mistakes. First, at z=0z=0 all source and detector times, frequencies, and masses agree, while DLD_L reduces to the local distance. Second, the phase product f dtf\,dt is invariant. Third, dimensionless combinations such as GMfG M f are preserved:

GMzfdet=GMsrcfsrc.GM_z f_{\rm det}=GM_{\rm src}f_{\rm src}.

A catalog source waveform can therefore be reused at any total mass and redshift by rescaling time and amplitude, provided matter scales or other dimensional source physics have not introduced extra structure. In the stationary-remnant limit, every quasinormal frequency is redshifted by the same factor and every damping time is stretched by it.

This page provides a parameter dictionary, not an inference procedure. A measured luminosity distance has an inclination correlation, and a host association or population model can supply information about zz; those empirical questions belong to gravitational-wave astronomy. The local orbital equations remain the responsibility of relativistic two-body dynamics.

A waveform analysis reports detector-frame component masses (m1,z,m2,z)=(45,30)M⊙(m_{1,z},m_{2,z})=(45,30)M_\odot, a detector frequency fdet=80 Hzf_{\rm det}=80\,\mathrm{Hz}, and a detector-frame interval Δtdet=15 ms\Delta t_{\rm det}=15\,\mathrm{ms}. An identified host has z=0.50z=0.50. Find the source-frame masses, mass ratio, corresponding source frequency, and source interval. Verify one invariant dimensionless product.

Solution

Here 1+z=1.51+z=1.5, so

(m1,src,m2,src)=(30,20)M⊙,q=4530=3020=1.5.(m_{1,\rm src},m_{2,\rm src})=(30,20)M_\odot, \qquad q=\frac{45}{30}=\frac{30}{20}=1.5.

Frequency and time transform oppositely:

fsrc=1.5(80 Hz)=120 Hz,Δtsrc=15 ms1.5=10 ms.f_{\rm src}=1.5(80\,\mathrm{Hz})=120\,\mathrm{Hz}, \qquad \Delta t_{\rm src}=\frac{15\,\mathrm{ms}}{1.5}=10\,\mathrm{ms}.

Using the total masses, Mz=75M⊙M_z=75M_\odot and Msrc=50M⊙M_{\rm src}=50M_\odot, the dimensionless frequency check is

GMzc3fdet=G(75M⊙)c3(80 Hz)=G(50M⊙)c3(120 Hz)=GMsrcc3fsrc≃0.02955.\frac{GM_z}{c^3}f_{\rm det} =\frac{G(75M_\odot)}{c^3}(80\,\mathrm{Hz}) =\frac{G(50M_\odot)}{c^3}(120\,\mathrm{Hz}) =\frac{GM_{\rm src}}{c^3}f_{\rm src} \simeq 0.02955.

The factor G/c3G/c^3 turns a mass into a time, so every displayed product is genuinely dimensionless. If one instead paired 75M⊙75M_\odot with 120 Hz120\,\mathrm{Hz}, the product would fail by the redshift factor and reveal a source/detector-frame mix-up.

  • Blanchet, Luc. “Post-Newtonian Theory for Gravitational Waves.” Living Reviews in Relativity 27 (2024) 4. DOI. Open PDF
  • Caprini, Chiara, and Daniel G. Figueroa. “Cosmological Backgrounds of Gravitational Waves.” Classical and Quantum Gravity 35 (2018) 163001. DOI. Open PDF
  • Hogg, David W. “Distance Measures in Cosmology.” arXiv:astro-ph/9905116 (1999). Abstract and PDF