The eikonal operator at arbitrary velocities I: the soft-radiation limit
Research output: Contribution to journal › Journal article › Research › peer-review
Standard
The eikonal operator at arbitrary velocities I : the soft-radiation limit. / Di Vecchia, Paolo; Heissenberg, Carlo; Russo, Rodolfo; Veneziano, Gabriele.
In: Journal of High Energy Physics, Vol. 2022, No. 7, 039, 07.07.2022.Research output: Contribution to journal › Journal article › Research › peer-review
Harvard
APA
Vancouver
Author
Bibtex
}
RIS
TY - JOUR
T1 - The eikonal operator at arbitrary velocities I
T2 - the soft-radiation limit
AU - Di Vecchia, Paolo
AU - Heissenberg, Carlo
AU - Russo, Rodolfo
AU - Veneziano, Gabriele
PY - 2022/7/7
Y1 - 2022/7/7
N2 - Observables related to the real part of the gravitational eikonal, such as the deflection angle and time delay, have been found so far to have a smooth post-Minkowskian (PM) expansion whose validity extends from the non-relativistic to the most extreme ultra-relativistic (UR) regime, which smoothly connects with massless particle collisions. To describe gravitational radiation, the eikonal phase has to be promoted to a unitary operator for which we motivate a proposal and start discussing properties in the soft-radiation limit. A convergent PM expansion is found to only hold below an UR bound (discussed in the GR literature in the seventies) above which a different expansion is instead needed implying, in general, some non-analyticity in Newton's constant. In this extreme UR regime soft radiative observables receive contributions only from gravitons and are therefore universal. This generalises the pattern discussed in [1] beyond the elastic case.
AB - Observables related to the real part of the gravitational eikonal, such as the deflection angle and time delay, have been found so far to have a smooth post-Minkowskian (PM) expansion whose validity extends from the non-relativistic to the most extreme ultra-relativistic (UR) regime, which smoothly connects with massless particle collisions. To describe gravitational radiation, the eikonal phase has to be promoted to a unitary operator for which we motivate a proposal and start discussing properties in the soft-radiation limit. A convergent PM expansion is found to only hold below an UR bound (discussed in the GR literature in the seventies) above which a different expansion is instead needed implying, in general, some non-analyticity in Newton's constant. In this extreme UR regime soft radiative observables receive contributions only from gravitons and are therefore universal. This generalises the pattern discussed in [1] beyond the elastic case.
KW - Black Holes
KW - Classical Theories of Gravity
KW - Scattering Amplitudes
KW - Supergravity Models
KW - GRAVITATIONAL-WAVES
KW - BREMSSTRAHLUNG
KW - GENERATION
KW - DERIVATION
KW - ENCOUNTERS
KW - PHOTONS
U2 - 10.1007/JHEP07(2022)039
DO - 10.1007/JHEP07(2022)039
M3 - Journal article
VL - 2022
JO - Journal of High Energy Physics (Online)
JF - Journal of High Energy Physics (Online)
SN - 1126-6708
IS - 7
M1 - 039
ER -
ID: 315265253