Abstract

We study the massive scalar field Sorkin-Johnston (SJ) Wightman function ${W}_{SJ}$ restricted to a flat 2D causal diamond $\mathcal{D}$ of linear dimension $L$. Our approach is two-pronged. In the first, we solve the central SJ eigenvalue problem explicitly in the small mass regime, up to order $(mL{)}^{4}$. This allows us to formally construct ${W}_{SJ}$ up to this order. Using a combination of analytical and numerical methods, we obtain expressions for ${W}_{SJ}$ both in the center and the corner of $\mathcal{D}$, to leading order. We find that in the center, ${W}_{SJ}$ is more like the massless Minkowski Wightman function ${W}_{0}^{\mathrm{mink}}$ than the massive one ${W}_{m}^{\mathrm{mink}}$, while in the corner it corresponds to that of the massive mirror ${W}_{m}^{\text{mirror}}$. In the second part, in order to explore larger masses, we perform numerical simulations using a causal set approximated by a flat 2D causal diamond. We find that in the center of the diamond the causal set SJ Wightman function ${W}_{SJ}^{c}$ resembles ${W}_{0}^{\mathrm{mink}}$ for small masses, as in the continuum, but beyond a critical value ${m}_{c}$ it resembles ${W}_{m}^{\mathrm{mink}}$, as expected. Our calculations suggest that unlike ${W}_{m}^{\mathrm{mink}}$, ${W}_{SJ}$ has a well-defined massless limit, which mimics the behavior of the Pauli Jordan function underlying the SJ construction. In the corner of the diamond, moreover, ${W}_{SJ}^{c}$ agrees with ${W}_{m}^{\text{mirror}}$ for all masses, and not, as might be expected, with the Rindler vacuum.

Highlights

  • The standard approach to quantum field theory is inherently observer dependent, as is evident from the Unruh effect for accelerating observers in Minkowski spacetime

  • We study the SJ vacuum for a massive free scalar field in the 2D

  • V we show the results of simulations of the causal set SJ vacuum for a range of masses

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Summary

INTRODUCTION

The standard approach to quantum field theory is inherently observer dependent, as is evident from the Unruh effect for accelerating observers in Minkowski spacetime. The calculations show that εcmenter; εcmorner contribute negligibly to WSJ both in the center and the corner This confirms that for a small mass WSJ corresponds to the massless Minkowski vacuum. The small mass regime agrees with our analytic calculation of WSJ in the center of the diamond and resembles mink 0. This means that it differs from Wmmink in the small mass regime. For a causal set that is approximated by de Sitter spacetime seems to behave very differently and in particular, does have a well defined m → 0 limit Understanding how these differences in behavior between the SJ and the standard vacua manifest themselves in the conditions Eq (2) should shed some light. In Appendix D we present a trick to get the 2D Rindler vacuum from the SJ prescription

THE SJ PRESCRIPTION
THE SPECTRUM OF THE PAULI JORDAN FUNCTION
Details of the calculations of SJ modes
Completeness of the eigenfunctions
The center
The corner
Numerical simulations for determining εm
THE MASSIVE SJ WIGHTMAN FUNCTION IN THE CAUSAL SET
DISCUSSION
Details of the calculations for the antisymmetric SJ modes
Details of the calculations for the symmetric SJ modes
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