Abstract

In this paper we investigate, within the standard model extension framework, the influence of Lorentz- and CPT-violating terms on gravitational quantum states of ultracold neutrons. Using a semiclassical wave packet, we derive the effective nonrelativistic Hamiltonian which describes the neutrons vertical motion by averaging the contributions from the perpendicular coordinates to the free falling axis. We compute the physical implications of the Lorentz- and CPT-violating terms on the spectra. The comparison of our results with those obtained in the GRANIT experiment leads to an upper bound for the symmetries-violation $c_{\mu\nu} ^{n}$ coefficients. We find that ultracold neutrons are sensitive to the $a _{i} ^{n}$ and $e _{i} ^{n}$ coefficients, which thus far are unbounded by experiments in the neutron sector. We propose two additional problems involving ultracold neutrons which could be relevant for improving our current bounds; namely, gravity-resonance-spectroscopy and neutron whispering gallery wave.

Highlights

  • One of the main challenges of modern physics is the search for a quantum theory of gravity (QTG)

  • Because of the good agreement between theory and experiment, neutron gravitational quantum states can be used for constraining deviations from the standard theory due to eventual new physical mechanisms

  • Since ultracold neutrons (UCNs) systems are nonrelativistic, we have used the nonrelativistic limit of the Dirac equation which can be obtained by using the FoldyWouthuysen procedure

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Summary

INTRODUCTION

One of the main challenges of modern physics is the search for a quantum theory of gravity (QTG). The recently observed gravitational quantum states of UCNs in the GRANIT experiments [24] offer an interesting opportunity of testing departures from both the neutrons quantum mechanical behavior and possible modifications of the local gravity field [25]. This fact motivates the investigation of SME effects on neutron gravitational quantum states, which is precisely the question we address here. V we briefly discuss two experiments involving UCNs, which can be used to improve our bound to the SME coefficients

LORENTZ VIOLATION IN A UNIFORM GRAVITATIONAL FIELD
EFFECTIVE HAMILTONIAN
ENERGY SHIFTS AND BOUNDS ON cnμν SME COEFFICIENTS
DISCUSSION AND OUTLOOK

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