Letter to the Editor

Using observations of distant quasars to constrain quantum gravity

¹ Department of Physics & Space SciencesFlorida Institute of Technology, 150 W. University Blvd., Melbourne, FL 32901, USA
e-mail: eperlman@fit.edu
² Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599, USA
e-mail: yjng@physics.unc.edu; wayne@physics.unc.edu
³ Monash Centre for Astrophysics, School of Physics, Monash University, PO Box 27, Clayton, Victoria 3800, Australia
e-mail: david.floyd@monash.edu

Received: 21 October 2011
Accepted: 13 November 2011

Abstract

Aims. The small-scale nature of spacetime can be tested with observations of distant quasars. We comment on a recent paper by Tamburini et al. (2011, A&A, 533, A71) which claims that Hubble Space Telescope (HST) observations of the most distant quasars place severe constraints on models of foamy spacetime.

Methods. If space is foamy on the Planck scale, photons emitted from distant objects will accumulate uncertainties in distance and propagation directions thus affecting the expected angular size of a compact object as a function of redshift. We discuss the geometry of foamy spacetime, and the appropriate distance measure for calculating the expected angular broadening. We also address the mechanics of carrying out such a test. We draw upon our previously published work on this subject, which carried out similar tests as Tamburini et al. and also went considerably beyond their work in several respects.

Results. When calculating the path taken by photons as they travel from a distant source to Earth, one must use the comoving distance rather than the luminosity distance. This then also becomes the appropriate distance to use when calculating the angular broadening expected in a distant source. The use of the wrong distance measure causes Tamburini et al. to overstate the constraints that can be placed on models of spacetime foam. In addition, we consider the impact of different ways of parametrizing and measuring the effects of spacetime foam. Given the variation of the shape of the point-spread function on the chip, as well as observation-specific factors, it is important to select carefully – and document – the comparison stars used as well as the methods used to compute the Strehl ratio.