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2011

Lensing Time Delays and Cosmological Complementarity

Linder, Eric V.

Understand

Time delays in strong gravitational lensing systems possess significant complementarity with distance measurements to determine the dark energy equation of state, as well as the matter density and Hubble constant.

Time delays are most useful when observations permit detailed lens modeling and variability studies, requiring high resolution imaging, long time monitoring, and rapid cadence.
We quantify the constraints possible between a sample of 150 such time delay lenses and a near term supernova program, such as might become available from an Antarctic telescope such as KDUST and the Dark Energy Survey.
Adding time delay data to supernovae plus cosmic microwave background information can improve the dark energy figure of merit by almost a factor 5 and determine the matter density \Omega_m to 0.004, Hubble constant h to 0.7%, and dark energy equation of state time variation w_a to 0.26, systematics permitting.

Built on

A.S. Bolton, S. Burles, L.V.E. Koopmans, T. Treu, R. Gavazzi, L.A. Moustakas, R. Wayth, D.J. Schlegel, Ap. J. 682, 964 (2008) [arXiv:0805.1931]
Original
1931
Earlier work this paper cites.
S. Refsdal, MNRAS 128, 307 (1964)
1964
Earlier work this paper cites.
K. Yamamoto, Y. Kadoya, T. Murata, T. Futamase, Prog. Theor. Phys. 106, 917 (2001) [arXiv:astro-ph/0110595]
2001
Earlier work this paper cites.
G.F. Lewis & R.A. Ibata, MNRAS 337, 26 (2002) [arXiv:astro-ph/0206425]
2002
Earlier work this paper cites.
http://snfactory.lbl.gov ; G. Aldering et al, SPIE 4836, 61 (2002)
2002
Earlier work this paper cites.
E.V. Linder, Phys. Rev. Lett. 90, 091301 (2003) [arXiv:astro-ph/0208512]
2003
Earlier work this paper cites.
E.V. Linder, Phys. Rev. D 68, 083503 (2003) [arXiv:astro-ph/0212301]
2003
Earlier work this paper cites.
E.V. Linder, Phys. Rev. D 70, 043534 (2004) [arXiv:astro-ph/0401433]
2004
Earlier work this paper cites.
E.V. Linder, Astropart. Phys. 24, 391 (2005) [arXiv:astro-ph/0508333]
2005
Earlier work this paper cites.
L. Knox, Phys. Rev. D 73, 023503 (2006) [arXiv:astro-ph/0503405]
2006
Earlier work this paper cites.