Abstract

We derive the response function for a comoving, pointlike Unruh-DeWitt particle detector coupled to a complex scalar field ϕ, in the (3 + 1)-dimensional cosmological de Sitter spacetime. The field-detector coupling is taken to be proportional to ϕ†ϕ. We address both conformally invariant and massless minimally coupled scalar field theories, respectively in the conformal and the Bunch-Davies vacuum. The response function integral for the massless minimal complex scalar, not surprisingly, shows divergences and accordingly we use suitable regularisation scheme to find out well behaved results. The regularised result also contains a de Sitter symmetry breaking logarithm, growing with the cosmological time. Possibility of extension of these results with the so called de Sitter α-vacua is discussed. While we find no apparent problem in computing the response function for a real scalar in these vacua, a complex scalar field is shown to contain some possible ambiguities in the detector response. The case of the minimal and nearly massless scalar field theory is also briefly discussed.

Highlights

  • Vacuum is thermal, there is no actual particle creation in this scenario

  • We derive the response function for a comoving, pointlike Unruh-DeWitt particle detector coupled to a complex scalar field φ, in the (3 + 1)-dimensional cosmological de Sitter spacetime

  • The response function integral for the massless minimal complex scalar, not surprisingly, shows divergences and we use suitable regularisation scheme to find out well behaved results

Read more

Summary

The setup

Following [1, 33, 34], we briefly review below the basic setup we use in this paper, for the sake of completeness. Since on the other hand the Wightman function does not represent propagation of the field, the same appearing in eq (2.11) can be interpreted as just an expectation value of the operator φ(x)φ(x ) with respect to the vacuum corresponding to the α modes. With this interpretation, we shall see below that at least for a real scalar field we can compute the response function in the α-vacua without any apparent ambiguity.

The conformal scalar
The minimally coupled massless scalar
Complex scalar in the Bunch-Davies vacuum
The minimally coupled massless complex scalar
The ambiguity of complex scalar field with α-vacua
The case of a nearly minimally coupled massless scalar
Discussions
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call