Abstract

The VIP-2 collaboration runs an apparatus in the Gran Sasso underground laboratories of the Italian Institute for Nuclear Physics (INFN) designed to search for anomalous X-rays from electron-atom interactions due to violations of the fundamental antisymmetry of multi-electron wavefunctions. The experiment implements the scheme first proposed by Ramberg and Snow, where a current source injects electrons into a metal strip (the experiment’s target). In this paper we describe the structure of a Monte Carlo program to simulate a new upgrade of the experiment, where the anomalous X-ray emission is modulated by an arbitrary time-varying input current. A novel feature of the simulation algorithm is that the Monte Carlo program is based on a mixture of analytical and numerical methods. We report preliminary, exploratory results on the expected detection rate for different modulations of the injected current; these results are a starting point on the way to optimize the modulation scheme and indicate a large potential improvement of the detection sensitivity.

Highlights

  • IntroductionTo the existence of neutron stars [2]

  • Since our aim is the estimate of the average signal, we adopt techniques that minimize the fluctuations of the Monte Carlo runs and boost computational efficiency

  • We detect a violation when we find that there is a statistically significant spectral peak that corresponds to a harmonic of the current modulation frequency

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Summary

Introduction

To the existence of neutron stars [2] As is it was clearly shown by Pauli [3], the principle lies at the crossroads of our most important theories, relativity and quantum physics, it is a very robust feature of relativistic Quantum Field Theory [4], and it is important to test its validity [5]. The VIP-2 experiment [6,7] (a followup of the VIP experiment [8]) tests the validity of the Pauli Exclusion Principle (PEP) for electrons—and the fundamental antisymmetry of the multi-electron wavefunctions—with the same conceptual setup first introduced by Ramberg and Snow in 1990 [9]. The final electron transitions in the electromagnetic cascade emit X-rays with energies that differ from those of the characteristic X-rays of the target material and provide a unique signature of the non-Paulian capture process (see [13] for a recent and precise theoretical determination of the energies of the characteristic X-rays of Cu)

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