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A Review of Searches for Evidence of Tachyons (2204.12017v5)

Published 26 Apr 2022 in hep-ph

Abstract: Here we review empirical evidence for the possible existence of tachyons, superluminal particles having m2 < 0: The review considers searches for new particles that might be tachyons, as well as evidence that neutrinos are tachyons from data which may have been gathered for other purposes. Much of the second half of the paper is devoted to the 3 + 3 neutrino model including a tachyonic mass state, which has empirical support from a variety of areas. Although this is primarily a review article, it contains several new results.

Citations (9)

Summary

  • The paper presents a detailed review of historical and modern experimental searches for tachyons and their implications in particle physics.
  • It examines key experiments such as OPERA, IceCube, and SN 1987A, highlighting neutrino anomalies and indirect signatures suggestive of tachyonic behavior.
  • The review proposes theoretical frameworks like the 3+3 model and Light Cone Reflection symmetry, outlining future directions for more sensitive tachyon detection.

A Review of Searches for Evidence of Tachyons

The paper "A Review of Searches for Evidence of Tachyons" by Robert Ehrlich offers a comprehensive exploration of the theoretical and experimental landscape associated with tachyons—hypothetical particles that travel faster than light and possess imaginary mass. Such particles challenge conventional physics, primarily due to potential violations of causality. This review not only revisits historical experiments but also considers neutrinos as potential tachyon candidates, presenting a nuanced discussion on the implications and current status of tachyon research.

Historical Context and Initial Searches

The conceptual foundation for tachyons was laid by Bilaniuk, Deshpande, and Sudarshan in the 1960s, who proposed the possible existence of superluminal particles. Feinberg extended this by suggesting tachyons could be excitations of a quantum field with imaginary mass. Early efforts to detect tachyons focused on both theoretical considerations and empirical searches for new particles that exhibited superluminal velocity or negative mass squared. Key predictions included the hypothetical emission of Cherenkov radiation in a vacuum, yet initial experiments largely resulted in null findings. These experiments, conducted using charged particle production and cosmic ray interactions, set stringent limits on tachyon production cross-sections and suggested their rarity, if they exist at all.

Neutrinos as Potential Tachyons

The notion that neutrinos might be tachyons gained traction due to the consistent reporting of neutrino mass squared values less than zero in several experimental results, albeit these were often dismissed as systematic errors. The review explores theoretical models, including the work of Chodos et al., who provided a framework for tachyonic neutrinos despite the challenges in formulating a complete quantum field theory. Recent theoretical motivations include potential violations of Lorentz invariance, for which neutrinos are prime candidates.

Empirical Evidence and Interpretations

Several key experiments are scrutinized for their potential to shed light on the tachyon hypothesis:

  • Superluminal Propagation Tests: The OPERA experiment's initial report of superluminal neutrino velocity sparked debate and led to numerous follow-up experiments, ultimately correcting the result to align with the speed of light after the identification of systematic errors.
  • IceCube and High-Energy Neutrino Observations: Potential signatures of superluminal neutrinos were investigated through their expected vacuum pair emission process at high energies. While initial claims suggested a spectral cut-off, further observations extended the detectable neutrino spectrum, leading to alternative interpretations involving Lorentz violation or multicomponent spectral origins.
  • Cosmic Ray Studies: The cosmic ray spectrum's features, notably the "knees" and "ankle," have been reinterpreted in the context of tachyonic neutrino decay chains, presenting a compelling if speculative support for specific mass values.
  • SN 1987A Neutrinos: The analysis of supernova neutrino data from SN 1987A presents a unique insight, suggesting consistent mass eigenstates related to arrival times and energies. This analysis supports the notion of tachyonic neutrinos within a multi-component mass model, yet remains contentious.

Theoretical Models and Implications

Ehrlich proposes distinct models, including the $3+3$ model that incorporates both tachyonic and conventional neutrino masses, attempting to reconcile anomalies in cosmic ray and supernova neutrino observations. Furthermore, the proposed Light Cone Reflection (LCR) symmetry suggests pairs of bradyonic and tachyonic neutrinos, offering a symmetric theoretical framework.

Future Directions and Challenges

The discussion emphasizes the necessity for further experiments, particularly those capable of resolving neutrino masses with unprecedented sensitivity, such as ongoing and future endeavors at the KATRIN facility and other direct mass measurements. Additionally, the potential role of tachyonic neutrinos in cosmology, particularly in explaining dark energy phenomena and Lorentz violations, remains a fertile ground for theoretical exploration.

While the experimental evidence for tachyons remains tenuous, the review underscores the need to remain open to unconventional ideas that challenge our understanding of particle physics and cosmology. A continued interplay between theoretical refinement and advanced experimental techniques will be crucial in resolving the longstanding enigma of tachyons.

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