RGE effects on new physics searches via gravitational waves
Katsuya Hashino, Daiki Ueda

TL;DR
This paper investigates how renormalization scale uncertainties affect the potential of gravitational wave observations to probe new physics, specifically within the SMEFT framework, emphasizing the importance of precise measurements of certain operators.
Contribution
It revisits Fisher matrix analyses incorporating renormalization scale uncertainties and assesses the impact of RGE running of SMEFT operators on gravitational wave signals.
Findings
GW observations can still probe SMEFT effects despite uncertainties.
Precise measurement of the $(H^{\u2293}H)^3$ operator is crucial for sensitivity.
RGE effects influence Higgs potential and GW spectrum predictions.
Abstract
Gravitational wave (GW) observations offer a promising probe of new physics associated with a first-order electroweak phase transition. Precision studies of the Higgs potential, including Fisher matrix analyses, have been extensively conducted in this context. However, significant theoretical uncertainties in the GW spectrum, particularly those due to renormalization scale dependence in the conventional daisy-resummed approach, have cast doubt on the reliability of such precision measurements. These uncertainties have been highlighted using the Standard Model Effective Field Theory (SMEFT) as a benchmark. To address these issues, we revisit Fisher matrix analyses based on the daisy-resummed approach, explicitly incorporating renormalization scale uncertainties. We then reassess the prospects for precise new physics measurements using GW observations. Adopting the SMEFT as a benchmark,…
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Pulsars and Gravitational Waves Research · Quantum Chromodynamics and Particle Interactions
