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Axion-like particles at future colliders

TLDR
In this paper, the reach of different proposed colliders is discussed, focusing on resonant ALP production, ALP production in the decay of heavy SM resonances, and associate ALP production with photons, Z bosons or Higgs bosons.
Abstract
Axion-like particles (ALPs) are pseudo Nambu–Goldstone bosons of spontaneously broken global symmetries in high-energy extensions of the Standard Model (SM). This makes them a prime target for future experiments aiming to discover new physics which addresses some of the open questions of the SM. While future high-precision experiments can discover ALPs with masses well below the GeV scale, heavier ALPs can be searched for at future high-energy lepton and hadron colliders. We discuss the reach of the different proposed colliders, focusing on resonant ALP production, ALP production in the decay of heavy SM resonances, and associate ALP production with photons, Z bosons or Higgs bosons. We consider the leading effective operators mediating interactions between the ALP and SM particles and discuss search strategies for ALPs decaying promptly as well as ALPs with delayed decays. Projections for the high-luminosity run of the LHC and its high-energy upgrade, CLIC, the future $$e^+e^-$$ ring-colliders CEPC and FCC-ee, the future pp colliders SPPC and FCC-hh, and for the MATHUSLA surface array are presented. We further discuss the constraining power of future measurements of electroweak precision parameters on the relevant ALP couplings.

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Axionlike Particles, Lepton-Flavor Violation, and a New Explanation of a μ and a e

TL;DR: Experimental constraints on ALPs with a single dominant lepton-flavor-violating coupling are discussed and allowing for one or more such couplings offers qualitatively new ways to explain the anomalies related to the magnetic moments of the muon or the electron.
Journal ArticleDOI

The low-energy effective theory of axions and ALPs

TL;DR: In this article, the authors studied the evolution of axion-like particle couplings from the new-physics scale to energies at and below the scale of electroweak symmetry breaking.
Journal ArticleDOI

Feebly-interacting particles: FIPs 2020 workshop report

P. Agrawal, +51 more
TL;DR: FIPs 2020 as mentioned in this paper was the first workshop dedicated to the physics of feebly-interacting particles and was held virtually from 31 August to 4 September 2020 at CERN, where experts from collider, beam dump, fixed target experiments, as well as from astrophysics, axions/ALPs searches, current/future neutrino experiments, and dark matter direct detection communities participated.
Journal ArticleDOI

The Forward Physics Facility at the High-Luminosity LHC

Jonathan L. Feng, +235 more
- 09 Mar 2022 - 
TL;DR: The Forward Physics Facility (FPF) as mentioned in this paper is a suite of experiments to probe standard model processes and search for physics beyond the standard model (BSM) beyond the acceptance of existing LHC experiments.
Journal ArticleDOI

Search for Axionlike and Scalar Particles with the NA64 Experiment.

TL;DR: A model-independent search for light scalar and pseudoscalar axionlike particles that couple to two photons by using the high-energy CERN SPS H4 electron beam is carried out, allowing for the probing of the a(s) parameter space, including those from generic axion models, inaccessible to previous experiments.
References
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TL;DR: In this article, it was pointed out that a global U(1) symmetry, introduced in order to preserve the parity and time-reversal invariance of strong interactions despite the effects of instantons, would lead to a neutral pseudoscalar boson, the "axion", with mass roughly of order 100 keV to 1 MeV.
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Problem of Strong $P$ and $T$ Invariance in the Presence of Instantons

TL;DR: In this article, the color gauge theory of strong interactions without arbitrary adjustment of parameters is analyzed and several possibilities are identified, including one which would give a remarkable new kind of very light, long-lived pseudoscalar boson.
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Cosmology of the invisible axion

TL;DR: In this article, the authors identify a new cosmological problem for models which solve the strong CP puzzle with an invisible axion, unrelated to the domain wall problem, and identify the energy density stored in the oscillations of the classical axion field does not dissipate rapidly; it exceeds the critical density needed to close the universe unless fa ⩽ 1012GeV wherefa is the axion decay constant.
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