QED positivity bounds
File(s)PhysRevD.103.125020.pdf (633.44 KB)
Published version
Author(s)
Alberte, Lasma
de Rham, Claudia
Jaitly, Sumer
Tolley, Andrew J
Type
Journal Article
Abstract
We apply positivity bounds directly to a
U
(
1
)
gauge theory with charged scalars and charged fermions, i.e., QED, minimally coupled to gravity. Assuming that the massless
t
-channel pole may be discarded, we show that the improved positivity bounds are violated unless new physics is introduced at the parametrically low scale
Λ
new
∼
(
e
m
M
Pl
)
1
/
2
, consistent with similar results for scalar field theories, far lower than the scale implied by the weak gravity conjecture. This is sharply contrasted with previous treatments which focus on the application of positivity bounds to the low energy gravitational Euler-Heisenberg effective theory only. We emphasize that the low cutoff is a consequence of applying the positivity bounds under the assumption that the pole may be discarded. We conjecture an alternative resolution that a small amount of negativity, consistent with decoupling limits, is allowed and is not in conflict with standard UV completions, including weakly coupled ones.
U
(
1
)
gauge theory with charged scalars and charged fermions, i.e., QED, minimally coupled to gravity. Assuming that the massless
t
-channel pole may be discarded, we show that the improved positivity bounds are violated unless new physics is introduced at the parametrically low scale
Λ
new
∼
(
e
m
M
Pl
)
1
/
2
, consistent with similar results for scalar field theories, far lower than the scale implied by the weak gravity conjecture. This is sharply contrasted with previous treatments which focus on the application of positivity bounds to the low energy gravitational Euler-Heisenberg effective theory only. We emphasize that the low cutoff is a consequence of applying the positivity bounds under the assumption that the pole may be discarded. We conjecture an alternative resolution that a small amount of negativity, consistent with decoupling limits, is allowed and is not in conflict with standard UV completions, including weakly coupled ones.
Date Issued
2021-06-22
Date Acceptance
2021-05-24
Citation
Physical Review D: Particles, Fields, Gravitation and Cosmology, 2021, 103 (12), pp.1-26
ISSN
1550-2368
Publisher
American Physical Society
Start Page
1
End Page
26
Journal / Book Title
Physical Review D: Particles, Fields, Gravitation and Cosmology
Volume
103
Issue
12
Copyright Statement
© 2021 The Author(s). Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
License URL
Sponsor
The Royal Society
Simons Foundation
Science and Technology Facilities Council (STFC)
European Research Council
Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council [2006-2012]
Identifier
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000664530200020&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
Grant Number
WM150044
PP00P2 123386
DE-SC0009946
555326
ST/P000762/1
724659 MassiveCosmo ERC-2016-COG
ST/T000791/1
ST/P000762/1
Subjects
Science & Technology
Physical Sciences
Astronomy & Astrophysics
Physics, Particles & Fields
Physics
Publication Status
Published
Article Number
ARTN 125020
Date Publish Online
2021-06-22