Cosmological parameter determination in free-form strong gravitational lens modelling

نویسندگان

  • M. Lubini
  • M. Sereno
  • J. Coles
  • P. Saha
چکیده

We develop a novel statistical strong-lensing approach to probe the cosmological parameters by exploiting multiple redshift image systems behind galaxies or galaxy clusters. The method relies on free-form mass inversion of strong lenses and does not need any additional information other than gravitational lensing. Since in free-form lensing the solution space is a high-dimensional convex polytope, we consider Bayesian model comparison analysis to infer the cosmological parameters. The volume of the solution space is taken as a tracer of the probability of the underlying cosmological assumption. In contrast to parametric mass inversions, our method accounts for the mass-sheet degeneracy, which implies a degeneracy between the steepness of the profile and the cosmological parameters. Parametric models typically break this degeneracy, introducing hidden priors to the analysis that contaminate the inference of the parameters. We test our method with synthetic lenses, showing that it is able to infer the assumed cosmological parameters. Applied to the Cluster Lensing And Supernova survey with Hubble (CLASH) clusters, the method might be competitive with other probes. DOI: https://doi.org/10.1093/mnras/stt2057 Posted at the Zurich Open Repository and Archive, University of Zurich ZORA URL: https://doi.org/10.5167/uzh-98139 Published Version Originally published at: Lubini, M; Sereno, M; Coles, J; Jetzer, P; Saha, P (2014). Cosmological parameter determination in free-form strong gravitational lens modelling. Monthly Notices of the Royal Astronomical Society, 437(3):2461-2470. DOI: https://doi.org/10.1093/mnras/stt2057 MNRAS 437, 2461–2470 (2014) doi:10.1093/mnras/stt2057 Advance Access publication 2013 November 30 Cosmological parameter determination in free-form strong gravitational lens modelling M. Lubini,1‹ M. Sereno,2,3 J. Coles,1 Ph. Jetzer1 and P. Saha1 1Institut für Theoretische Physik, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland 2Dipartimento di Scienza Applicata e Tecnologia, Politecnico di Torino, Corso Duca degli Abruzzi 24, I-10129 Torino, Italia 3INFN, Sezione di Torino, Via Pietro Giuria 1, I-10125 Torino, Italia Accepted 2013 October 23. Received 2013 September 24; in original form 2013 April 26

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Galaxy-scale Strong Lensing Tests of Gravity and Geometric Cosmology: Constraints and Systematic Limitations1

Galaxy-scale strong gravitational lenses with measured stellar velocity dispersions allow a test of the weakfield metric on kiloparsec scales and a geometric measurement of the cosmological distance–redshift relation, provided that the mass-dynamical structure of the lensing galaxies can be indepently constrained to a sufficient degree. We combine data on 53 galaxy-scale strong lenses from the ...

متن کامل

The cosmological lens equation and the equivalent single-plane gravitational lens

The gravitational lens equation resulting from a single (non-linear) mass concentration (the main lens) plus inhomogeneities of the large-scale structure is shown to be strictly equivalent to the single-plane gravitational lens equation without the cosmological perturbations. The deflection potential (and, by applying the Poisson equation, also the mass distribution) of the equivalent single-pl...

متن کامل

Galaxy-scale Strong-lensing Tests of Gravity and Geometric Cosmology: Constraints and Systematic Limitations

Galaxy-scale strong gravitational lenses with measured stellar velocity dispersions allow a test of the weak-field metric on kiloparsec scales and a geometric measurement of the cosmological distance–redshift relation, provided that the mass-dynamical structure of the lensing galaxies can be independently constrained to a sufficient degree. We combine data on 53 galaxy-scale strong lenses from ...

متن کامل

The age of the universe and the mass of stars by gravitational lensing

We present a simultaneous analysis of 10 galaxy lenses having time delay measurements. For each lens, wederive a detailed free-form mass map, with uncertainties, and with the additional requirement of a shared valueof the Hubble parameter across all the lenses. We test the prior involved in the lens reconstruction against agalaxy-formation simulation. Assuming a concordance cosmolog...

متن کامل

Noise in Strong Lensing Cosmography

Giant arcs in strong lensing galaxy clusters can provide a purely geometric determination of cosmological parameters, such as the dark energy density and equation of state. We investigate sources of noise in cosmography with giant arcs, focusing in particular on errors induced by density fluctuations along the line-of-sight, and errors caused by modeling uncertainties. We estimate parameter err...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2017