A scalar cosmological perturbation at fixed wavevector carries no helicity or distinguished transverse direction. Its metric and scalar sources are unchanged by rotations around , and the scalar baryon peculiar velocity is longitudinal. With scalar initial conditions, rotational invariance of the linear evolution therefore makes a function only of . Expand it using the stated normalization, without an extra factor:In the Thomson kernel, . The spherical harmonic addition theorem and Orthogonality of Legendre polynomials giveOnly the monopole and quadrupole survive; the quadrupole's gives the angular scattering integralThis also explains why an isotropic distribution has zero net collision term.
The streaming term and the Legendre polynomial recurrence relation yield, after division by , . With , the velocity collision source is in the dipole equation; the gravitational gradient source is . Therefore the photon Boltzmann hierarchy isSet the absent contribution to zero. This is algebraically the printed hierarchy. In particular,Since , these collision terms damp the nonzero multipoles and drive the dipole to . The latter sign follows from the paper's velocity and conventions, not a reversed physical photon velocity.
In the tight-coupling approximation, the Thomson-scattering rate is much faster than both spatial streaming and cosmological evolution: and . Frequent scattering locks the photon and baryon velocities and suppresses higher angular multipoles. The photon dipole is leading order, while the photon quadrupole is first order in the mean-free-time expansion.
Use the quadrupole equation. Its time derivative is smaller than its collision term by an additional expansion parameter, and starts one order beyond . The leading balance is thereforeThus for the temperature-only collision operator supplied here,The temperature-only tight-coupling quadrupole is not numerically interchangeable with a hierarchy that includes polarization feedback. The latter changes the leading collision coefficient and gives the existing photon quadrupole in tight coupling with polarization instead. Here the stated temperature-only approximation is the one being expanded.
For , scalar axisymmetry leaves only in the photon quadrupole: with the normalization used above. The two spin-weighted spherical harmonics satisfy . Translation from last scattering supplies . Thus the two helicity combinations have the same scalar source:where is a common normalization constant independent of . In this meridian polarization basis the scalar contribution has ; this does not mean that every rotated polarization basis has zero .
Apply the spin-raising and lowering operators to an axisymmetric scalar potential . The first action is . In the second action, the intermediate spin is respectively or ; both giveIt follows thatSubtracting the two equations gives . The possible affine consists solely of the unobservable kernel of the twice-applied spin operators. Defining polarization potentials to have no such components sets the physical scalar B mode to zero, . This is the low-multipole kernel of polarization potentials, not a physical dipole polarization.
For the remaining equation integrates to . Remove the same monopole/dipole kernel and use the plane-wave expansion. Thus the scalar E-mode radial projection isThe overall minus sign is absorbed in the stated proportionality constant. Although the unprojected antiderivative has , its divergent monopole and dipole pieces are discarded; the physical limit is finite because .
The temperature-only tight-coupling quadrupole is suppressed by . For regular superhorizon scalar modes, the photon dipole is itself proportional to , so the recombination quadrupole and the resulting polarization are especially small at large angular scales. Last-scattering polarization is generated by the small departure from perfect tight coupling, not by an isotropic monopole. Reionization can generate a separate large-angle signal after recombination and is absent from the instantaneous-last-scattering approximation here. The no-B-mode conclusion applies to linear scalar sources; it does not include tensor sources or conversion by lensing.
Articles by others on the same topic
There are currently no matching articles.