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Photon Masses in the Landscape and the Swampland

Published 29 Aug 2018 in hep-th and hep-ph | (1808.09966v2)

Abstract: In effective quantum field theory, a spin-1 vector boson can have a technically natural small mass that does not originate from the Higgs mechanism. For such theories, which may be written in St\"uckelberg form, there is no point in field space at which the mass is exactly zero. I argue that quantum gravity differs from, and constrains, effective field theory: arbitrarily small St\"uckelberg masses are forbidden. In particular, the limit in which the mass goes to zero lies at infinite distance in field space, and this distance is correlated with a tower of modes becoming light according to the Swampland Distance Conjecture. Application of Tower or Sublattice variants of the Weak Gravity Conjecture makes this statement more precise: for a spin-1 vector boson with coupling constant $e$ and St\"uckelberg mass $m$, local quantum field theory breaks down at energies at or below $\Lambda_{\rm UV} = \min((m M_{\rm Pl}/e){1/2}, e{1/3} M_{\rm Pl})$. Combined with phenomenological constraints, this argument implies that the Standard Model photon must be exactly massless. It also implies that much of the parameter space for light dark photons, which are the target of many experimental searches, is compatible only with Higgs and not St\"uckelberg mass terms. This significantly affects the experimental limits and cosmological histories of such theories. I explain various caveats and weak points of the arguments, including loopholes that could be targets for model-building.

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Summary

Photon Masses in the Landscape and the Swampland: A Critical Examination

Matthew Reece's paper explores the potential implications of a nonzero photon mass within the framework of quantum gravity, juxtaposing two theoretical paradigms: the Higgs mechanism and the Stückelberg mechanism. The discourse delves into effective quantum field theory (QFT) and the constraints that quantum gravity might impose on such theories, particularly concerning the existence and property of massive spin-1 particles, like photons.

The paper argues that while effective QFT allows for the formulation of a massive photon, especially through the Stückelberg mechanism, quantum gravity could prohibit such possibilities due to specific swampland conjectures. These conjectures suggest that effective field theories lacking ultraviolet (UV) completions—which adhere to the requirements of a consistent quantum gravity—reside in the so-called "swampland." Key swampland conjectures such as the Weak Gravity Conjecture (WGC) and the Swampland Distance Conjecture (SDC) play pivotal roles in constraining the mass parameters in these theories.

Photon Mass in Effective Field Theories

In effective QFTs, photons can be massless due to gauge invariance. However, Reece critiques the dogmatic adherence to gauge invariance in declaring photons massless. He draws a parallel to other historical cases such as neutrino masses and cosmological constants which were presumed zero until empirical evidence suggested otherwise. This makes the question of whether the photon possesses a tiny yet nonzero mass legitimate within QFT.

Constraints on photon mass largely stem from astrological phenomena, for instance, bounds derived from Fast Radio Bursts (FRBs) and giant planetary magnetic fields like those of Jupiter. These yield upper limitations on potential photon mass but do not conclusively negate a small mass hypothesis.

Quantum Gravity's Take: The Higgs vs. the Stückelberg Approach

Reece further analyzes these possibilities through the lens of quantum gravity. In this context, the Higgs mechanism, where massless vector bosons acquire mass, is distinct from the Stückelberg mechanism, where bosons achieve mass through an external gauge symmetry invoked by scalar fields. Both the Higgs and Stückelberg mechanisms are technically natural when radiative corrections are considered. However, the distinction rests in the validity span in field space between the two: the Higgs massless point in field space lies at finite distance, whereas, for the Stückelberg scenario, it is at an infinite distance, suggesting sundered consistency with quantum gravity principles.

The crux is that the infinite distance in field space—central to the Stückelberg scenario—when translated into swampland parlance, indicates a breakdown of local effective QFT owing to a possible tower of modes becoming light, as implied by the SDC. In stricter terms, the photon mass in the Stückelberg mechanism leads to a field theory only valid below a UV cutoff energy significantly lower than the Planck scale.

Implications and Theoretical Speculations

Reece implies a stronger theoretical preference for Higgs mechanism-induced photons, arguing that properties unique to Stückelberg mass generation, such as a UV cutoff determined by constraints like the WGC, might render Stückelberg mass generation infeasible. The posited bounds are tight enough to restrict scenarios where photon mass via the Higgs mechanism, despite being finely tuned, remains consistent and theoretically tenable within proposed phenomenological constraints.

The conclusions drawn extend beyond standard-model photons to "dark photons," which exist speculatively in numerous theoretical models, particularly those concerning dark matter and dark forces. Reece challenges much of the parameter space examined experimentally for dark photon dark matter, especially in scenarios where Stückelberg mass considerations apply. The results unlock paths for further exploration into Higgs mechanism alternatives or stringent empirical searches to radically validate or refute these propositions.

Reece urges continued phenomenological investigation—a task for high energy experimentations—not just for substantively challenging these conjectures, but also potentially necessitating reframing or model-building adaptations should empirical intentions uncover any photon mass.

Conclusion

Matthew Reece's inquiry marks a pivotal intersection of fundamental physics and emerging astrophysical evidence, where quantum gravity could inform crucial limits on particle mass. The presumptions aligned with swampland conjectures could reshape the landscape of viable theories, prompting either tightened phenomenological controls or new physics, especially in the pursuit of so-called "naturalness" in high-energy physics. This analysis emphasizes the vital role of integrating quantum gravitational principles with traditional particle physics paradigms—a critical frontier for contemporary research.

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