ePrints@IIScePrints@IISc Home | About | Browse | Latest Additions | Advanced Search | Contact | Help

Reconstructing the properties of dark energy using standard sirens

Arabsalmani, Maryam and Sahni, Varun and Saini, Tarun Deep (2013) Reconstructing the properties of dark energy using standard sirens. In: PHYSICAL REVIEW D, 87 (8).

[img] PDF
phy_rev_87_8_083001_2013.pdf - Published Version
Restricted to Registered users only

Download (827kB) | Request a copy
Official URL: http://dx.doi.org/10.1103/PhysRevD.87.083001


Future space-based gravity wave (GW) experiments such as the Big Bang Observatory (BBO), with their excellent projected, one sigma angular resolution, will measure the luminosity distance to a large number of GW sources to high precision, and the redshift of the single galaxies in the narrow solid angles towards the sources will provide the redshifts of the gravity wave sources. One sigma BBO beams contain the actual source in only 68% of the cases; the beams that do not contain the source may contain a spurious single galaxy, leading to misidentification. To increase the probability of the source falling within the beam, larger beams have to be considered, decreasing the chances of finding single galaxies in the beams. Saini et al. T.D. Saini, S.K. Sethi, and V. Sahni, Phys. Rev. D 81, 103009 (2010)] argued, largely analytically, that identifying even a small number of GW source galaxies furnishes a rough distance-redshift relation, which could be used to further resolve sources that have multiple objects in the angular beam. In this work we further develop this idea by introducing a self-calibrating iterative scheme which works in conjunction with Monte Carlo simulations to determine the luminosity distance to GW sources with progressively greater accuracy. This iterative scheme allows one to determine the equation of state of dark energy to within an accuracy of a few percent for a gravity wave experiment possessing a beam width an order of magnitude larger than BBO (and therefore having a far poorer angular resolution). This is achieved with no prior information about the nature of dark energy from other data sets such as type Ia supernovae, baryon acoustic oscillations, cosmic microwave background, etc. DOI:10.1103/PhysRevD.87.083001

Item Type: Journal Article
Additional Information: Copyright for this article belongs to the AMER PHYSICAL SOC, USA.
Department/Centre: Division of Physical & Mathematical Sciences > Physics
Date Deposited: 20 May 2013 07:07
Last Modified: 20 May 2013 07:07
URI: http://eprints.iisc.ac.in/id/eprint/46485

Actions (login required)

View Item View Item