The sky remembers everything: Celestial amplitude, shadow and OPE in quadratic EFT of gravity

In this paper, we compute the celestial amplitude arising from higher curvature corrections to Einstein gravity, incorporating phase dressing. The inclusion of such corrections leads to effective modifications of the theory’s ultraviolet (UV) behaviour. In the eikonal limit, we find that, in contrast to Einstein’s gravity, where the u <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>u</mml:mi> </mml:math> and s <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>s</mml:mi> </mml:math> -channel contributions cancel, these contributions remain non-vanishing in the presence of higher curvature terms. We examine the analytic structure of the resulting amplitude and derive a dispersion relation for the phase-dressed eikonal amplitude in quadratic gravity. Furthermore, we investigate the celestial conformal block expansion of the Mellin-transformed conformal shadow amplitude within the framework of celestial conformal field theory (CCFT). As a consequence, we compute the corresponding operator product expansion (OPE) coefficients using the Burchnall-Chaundy expansion. In addition, we evaluate the OPE via the Euclidean OPE inversion formula across various kinematic channels and comment on its applicability and implications. Finally, we briefly explore the Carrollian amplitude associated with the corresponding quadratic EFT.

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Publication Details

Journal
SciPost Physics
Published
2025-08-15
DOI
https://doi.org/10.21468/scipostphys.19.2.041
Citations
3
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
5.61

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article

The sky remembers everything: Celestial amplitude, shadow and OPE in quadratic EFT of gravity

Sounak Pal, Arpan Bhattacharyya, Saptaswa Ghosh
3 citations
SciPost Physics
Black Holes and Theoretical Physics
5.61
article

The sky remembers everything: Celestial amplitude, shadow and OPE in quadratic EFT of gravity

Sounak Pal, Arpan Bhattacharyya, Saptaswa Ghosh
article en
3 citations

Abstract

In this paper, we compute the celestial amplitude arising from higher curvature corrections to Einstein gravity, incorporating phase dressing. The inclusion of such corrections leads to effective modifications of the theory’s ultraviolet (UV) behaviour. In the eikonal limit, we find that, in contrast to Einstein’s gravity, where the u <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>u</mml:mi> </mml:math> and s <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>s</mml:mi> </mml:math> -channel contributions cancel, these contributions remain non-vanishing in the presence of higher curvature terms. We examine the analytic structure of the resulting amplitude and derive a dispersion relation for the phase-dressed eikonal amplitude in quadratic gravity. Furthermore, we investigate the celestial conformal block expansion of the Mellin-transformed conformal shadow amplitude within the framework of celestial conformal field theory (CCFT). As a consequence, we compute the corresponding operator product expansion (OPE) coefficients using the Burchnall-Chaundy expansion. In addition, we evaluate the OPE via the Euclidean OPE inversion formula across various kinematic channels and comment on its applicability and implications. Finally, we briefly explore the Carrollian amplitude associated with the corresponding quadratic EFT.

SciPost PhysicsVol. 19(2)
Indian Institute of Technology Gandhinagar (IN)
Arthritis National Research Foundation, New York University Abu Dhabi, Indian Academy of Sciences, York University, Department of Science and Technology, Ministry of Science and Technology, India, Ministry of Education, India, Birla Institute of Technology and Science, Pilani
Openalex Percentile: Top 5%
Black Holes and Theoretical Physics
5.61
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