Neutrino and photon lensing by black holes: radiative lens equations and post-Newtonian contributions

Marta Dell'Atti, Claudio Coriano', Luigi Delle Rose, Antonio Costantini

Research output: Contribution to journalArticlepeer-review

Abstract

We extend a previous phenomenological analysis of photon lensing in an external gravitational background to the case of a massless neutrino, and propose a method to incorporate radiative effects in the classical lens equations of neutrinos and photons. The study is performed for a Schwarzschild metric, generated by a point-like source, and expanded in the Newtonian potential at first order. We use a semiclassical approach, where the perturbative corrections to neutrino scattering, evaluated at one-loop in the Standard Model, are compared with the Einstein formula for the deflection using an impact parameter formulation. For this purpose, we use the renormalized expression of the graviton/fermion/fermion vertex presented in previous studies. We show the agreement between the classical and the semiclassical formulations, for values of the impact parameter b h of the neutrinos of the order of b h ∼ 20, measured in units of the Schwarzschild radius. The analysis is then extended with the inclusion of the post Newtonian corrections in the external gravity field, showing that this extension finds application in the case of the scattering of a neutrino/photon off a primordial black hole. The energy dependence of the deflection, generated by the quantum corrections, is then combined with the standard formulation of the classical lens equations. We illustrate our approach by detailed numerical studies, using as a reference both the thin lens and the Virbhadra-Ellis lens.
Original languageEnglish
Number of pages58
JournalJournal of High Energy Physics
Volume07
Issue number160
DOIs
Publication statusPublished - 29 Jul 2015

Keywords

  • black holes
  • neutrino physics
  • standard model

Fingerprint

Dive into the research topics of 'Neutrino and photon lensing by black holes: radiative lens equations and post-Newtonian contributions'. Together they form a unique fingerprint.

Cite this