The eikonal operator at arbitrary velocities I: the soft-radiation limit

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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 journalJournal articleResearchpeer-review

Harvard

Di Vecchia, P, Heissenberg, C, Russo, R & Veneziano, G 2022, 'The eikonal operator at arbitrary velocities I: the soft-radiation limit', Journal of High Energy Physics, vol. 2022, no. 7, 039. https://doi.org/10.1007/JHEP07(2022)039

APA

Di Vecchia, P., Heissenberg, C., Russo, R., & Veneziano, G. (2022). The eikonal operator at arbitrary velocities I: the soft-radiation limit. Journal of High Energy Physics, 2022(7), [039]. https://doi.org/10.1007/JHEP07(2022)039

Vancouver

Di Vecchia P, Heissenberg C, Russo R, Veneziano G. The eikonal operator at arbitrary velocities I: the soft-radiation limit. Journal of High Energy Physics. 2022 Jul 7;2022(7). 039. https://doi.org/10.1007/JHEP07(2022)039

Author

Di Vecchia, Paolo ; Heissenberg, Carlo ; Russo, Rodolfo ; Veneziano, Gabriele. / The eikonal operator at arbitrary velocities I : the soft-radiation limit. In: Journal of High Energy Physics. 2022 ; Vol. 2022, No. 7.

Bibtex

@article{618f4a4a722343309a63833e5018ef38,
title = "The eikonal operator at arbitrary velocities I: the soft-radiation limit",
abstract = "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.",
keywords = "Black Holes, Classical Theories of Gravity, Scattering Amplitudes, Supergravity Models, GRAVITATIONAL-WAVES, BREMSSTRAHLUNG, GENERATION, DERIVATION, ENCOUNTERS, PHOTONS",
author = "{Di Vecchia}, Paolo and Carlo Heissenberg and Rodolfo Russo and Gabriele Veneziano",
year = "2022",
month = jul,
day = "7",
doi = "10.1007/JHEP07(2022)039",
language = "English",
volume = "2022",
journal = "Journal of High Energy Physics (Online)",
issn = "1126-6708",
publisher = "Springer",
number = "7",

}

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