Strong Gravitational Lensing Time Delay Statistics and the Density Profile of Dark Halos

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

27 pages, 9 figures, accepted for publication in ApJ

Scientific paper

10.1086/339064

The distribution of differential time delays \Delta t between images produced by strong gravitational lensing contains information on the mass distributions in the lensing objects as well as on cosmological parameters such as H_0. We derive an explicit expression for the conditional probability distribution function of time delays P(\Delta t|\theta), given an image separation between multiple images \theta, and related statistics. We consider lensing halos described by the singular isothermal sphere (SIS) approximation and by its generalization as proposed by Navarro, Frenk, & White (NFW) which has a density profile \rho \propto r^{-\alpha} in the innermost region. The time delay distribution is very sensitive to these profiles; steeper inner slopes tend to produce larger time delays. For example, if H_0=70 km/s/Mpc, a \Lambda-dominated cosmology and a source redshift z_S=1.27 are assumed, lenses with \theta=5'' produce a time delay of \Delta t[yr]=1.5^{+1.7}_{-0.9}, 0.39^{+0.37}_{-0.22}, 0.15^{+0.11}_{-0.09}, and 0.071^{+0.054}_{-0.038} (50% confidence interval), for SIS, generalized NFW with \alpha=1.5, \alpha=1.0, and \alpha=0.5, respectively. At a fixed image separation, the time delay is determined by the difference in the lensing potential between the position of the two images, which typically occur at different impact parameters. Although the values of \Delta t are proportional to the inverse of H_0, P(\Delta t|\theta) is rather insensitive to all other cosmological model parameters, source redshifts, magnification biases and so on. A knowledge of P(\Delta t|\theta) will also be useful in designing the observing program of future large scale synoptic variability surveys and for evaluating possible selection biases operating against large splitting lens systems.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Strong Gravitational Lensing Time Delay Statistics and the Density Profile of Dark Halos does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Strong Gravitational Lensing Time Delay Statistics and the Density Profile of Dark Halos, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Strong Gravitational Lensing Time Delay Statistics and the Density Profile of Dark Halos will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-371740

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.