Dark matter and weak signals of quantum spacetime

Sergio Doplicher, Klaus Fredenhagen, Gerardo Morsella, and Nicola Pinamonti
Phys. Rev. D 95, 065009 – Published 13 March 2017

Abstract

In physically motivated models of quantum spacetime, a U(1) gauge theory turns into a U() gauge theory; hence, free classical electrodynamics is no longer free and neutral fields may have electromagnetic interactions. We discuss the last point for scalar fields, as a way to possibly describe dark matter; we have in mind the gravitational collapse of binary systems or future applications to self-gravitating Bose-Einstein condensates as possible sources of evidence of quantum gravitational phenomena. The effects considered so far, however, seem too faint to be detectable at present.

  • Received 29 December 2016

DOI:https://doi.org/10.1103/PhysRevD.95.065009

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsGravitation, Cosmology & Astrophysics

Authors & Affiliations

Sergio Doplicher1,*, Klaus Fredenhagen2,†, Gerardo Morsella3,‡, and Nicola Pinamonti4,§

  • 1Dipartimento di Matematica, Università di Roma “La Sapienza”, Piazzale Aldo Moro 5, I-00185 Roma, Italy
  • 2II Institut für Theoretische Physik, Universität Hamburg, D-22761 Hamburg, Germany
  • 3Dipartimento di Matematica, Università di Roma “Tor Vergata”, Via della Ricerca Scientifica, I-00133 Roma, Italy
  • 4Dipartimento di Matematica, Università di Genova, Via Dodecaneso 35, I-16146 Genova, Italy, and INFN Sezione di Genova, Genova, Italy

  • *dopliche@mat.uniroma1.it
  • klaus.fredenhagen@desy.de
  • morsella@mat.uniroma2.it
  • §pinamont@dima.unige.it

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Issue

Vol. 95, Iss. 6 — 15 March 2017

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