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Conformally Soft Photons and Gravitons

Laura Donnay, Andrea Puhm, Andrew Strominger

TL;DR

Reframes the 4D S-matrix as a celestial CFT correlator on the sphere at null infinity and introduces conformally soft photons and gravitons with h or hbar equal to zero. It constructs Goldstone modes for large gauge transformations and BMS supertranslations, together with logarithmic partners that generate celestial currents, including a U(1) Kac-Moody current and a supertranslation current. The work derives canonical pairings between Goldstone and conformally soft modes, develops their OPE and shadow structures, and connects soft theorems to celestial symmetry algebras and a 2D stress tensor on the celestial sphere. These results provide a concrete framework linking asymptotic symmetries to 4D scattering data and suggest strong constraints on celestial correlators in quantum gravity.

Abstract

The four-dimensional $S$-matrix is reconsidered as a correlator on the celestial sphere at null infinity. Asymptotic particle states can be characterized by the point at which they enter or exit the celestial sphere as well as their $SL(2,\mathbb C)$ Lorentz quantum numbers: namely their conformal scaling dimension and spin $h\pm \bar h$ instead of the energy and momentum. This characterization precludes the notion of a soft particle whose energy is taken to zero. We propose it should be replaced by the notion of a conformally soft particle with $h=0$ or $\bar h=0$. For photons we explicitly construct conformally soft $SL(2,\mathbb C)$ currents with dimensions $(1,0)$ and identify them with the generator of a $U(1)$ Kac-Moody symmetry on the celestial sphere. For gravity the generator of celestial conformal symmetry is constructed from a $(2,0)$ $SL(2,\mathbb C)$ primary wavefunction. Interestingly, BMS supertranslations are generated by a spin-one weight $(\frac{3}{2},\frac{1}{2})$ operator, which nevertheless shares holomorphic characteristics of a conformally soft operator. This is because the right hand side of its OPE with a weight $(h,\bar h)$ operator ${\cal O}_{h,\bar h}$ involves the shifted operator ${\cal O}_{h+\frac{1}{2},\bar h+ \frac{1}{2}}$. This OPE relation looks quite unusual from the celestial CFT$_2$ perspective but is equivalent to the leading soft graviton theorem and may usefully constrain celestial correlators in quantum gravity.

Conformally Soft Photons and Gravitons

TL;DR

Reframes the 4D S-matrix as a celestial CFT correlator on the sphere at null infinity and introduces conformally soft photons and gravitons with h or hbar equal to zero. It constructs Goldstone modes for large gauge transformations and BMS supertranslations, together with logarithmic partners that generate celestial currents, including a U(1) Kac-Moody current and a supertranslation current. The work derives canonical pairings between Goldstone and conformally soft modes, develops their OPE and shadow structures, and connects soft theorems to celestial symmetry algebras and a 2D stress tensor on the celestial sphere. These results provide a concrete framework linking asymptotic symmetries to 4D scattering data and suggest strong constraints on celestial correlators in quantum gravity.

Abstract

The four-dimensional -matrix is reconsidered as a correlator on the celestial sphere at null infinity. Asymptotic particle states can be characterized by the point at which they enter or exit the celestial sphere as well as their Lorentz quantum numbers: namely their conformal scaling dimension and spin instead of the energy and momentum. This characterization precludes the notion of a soft particle whose energy is taken to zero. We propose it should be replaced by the notion of a conformally soft particle with or . For photons we explicitly construct conformally soft currents with dimensions and identify them with the generator of a Kac-Moody symmetry on the celestial sphere. For gravity the generator of celestial conformal symmetry is constructed from a primary wavefunction. Interestingly, BMS supertranslations are generated by a spin-one weight operator, which nevertheless shares holomorphic characteristics of a conformally soft operator. This is because the right hand side of its OPE with a weight operator involves the shifted operator . This OPE relation looks quite unusual from the celestial CFT perspective but is equivalent to the leading soft graviton theorem and may usefully constrain celestial correlators in quantum gravity.

Paper Structure

This paper contains 23 sections, 107 equations, 1 figure.

Figures (1)

  • Figure 1: Wavefunction of the conformally soft photon. A radiative shock wave with initial data at $v=0$ emerges from past null infinity ${\mathcal{I}}^-$, impinges on the origin, and reemerges at $u=0$ at future null infinity ${\mathcal{I}}^+$. Coulombic fields are produced by and confined to the future of the incoming shockwave, and annihilated by and confined to the past of the outgoing shock wave.