Quantization of fluctuations in deformed special relativity: The two-point function and beyond

Giulia Gubitosi, Michele Arzano, and João Magueijo
Phys. Rev. D 93, 065027 – Published 11 March 2016

Abstract

We show that the two-point function of a quantum field theory with de Sitter momentum space (herein called DSR) can be expressed as the product of a standard delta function and an energy-dependent factor. The proportionality to a standard delta function is a nontrivial result valid in any theory without a preferred frame and relies crucially on the on-shellness condition. Different theories are distinguished by the specific form of the energy-dependent proportionality factor. Applied to models exhibiting running of the dimensionality of space, this result is essential in proving that vacuum fluctuations are generally scale invariant at high energies whenever there is running to two dimensions. This is equally true for theories with and without a preferred frame, with differences arising only as we consider higher order correlators. Specifically, the three-point function of DSR has a unique structure of “open triangles,” as shown here.

  • Figure
  • Received 10 November 2015

DOI:https://doi.org/10.1103/PhysRevD.93.065027

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

Giulia Gubitosi1, Michele Arzano2, and João Magueijo1

  • 1Theoretical Physics, Blackett Laboratory, Imperial College, London SW7 2BZ, United Kingdom
  • 2Dipartimento di Fisica, Università “La Sapienza” and Sezione Roma1 Istituto Nazionale di Fisica Nucleare (INFN), Piazzale Aldo Moro 2, 00185 Rome, Italy

See Also

Vacuum fluctuations in theories with deformed dispersion relations

Michele Arzano, Giulia Gubitosi, João Magueijo, and Giovanni Amelino-Camelia
Phys. Rev. D 91, 125031 (2015)

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Vol. 93, Iss. 6 — 15 March 2016

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