corner
corner

Phys. Rev. D 77, 123509 (2008) [8 pages]

Search for cosmic strings in the Great Observatories Origins Deep Survey

Download: PDF (1,007 kB) Buy this article Export: BibTeX or EndNote (RIS)

J. L. Christiansen1,*, E. Albin1, and K. A. James1
1Department of Physics, California Polytechnic State University, San Luis Obispo, California 93407, USA

J. Goldman2
2Department of Physics, Faculty of Science, National University of Singapore, Singapore, 117542

D. Maruyama3
3Department of Physics, University of California, Berkeley, California 94720, USA

G. F. Smoot4
4Lawrence Berkeley National Laboratory, Space Sciences Laboratory and Department of Physics, University of California, Berkeley, California 94720, USA

Received 26 February 2008; revised 18 May 2008; published 9 June 2008

We search Hubble Space Telescope Treasury Program images collected as part of the Great Observatories Origins Deep Survey for pairs of galaxies consistent with the gravitational lensing signature of a cosmic string. Our technique includes estimates of the efficiency for finding the lensed galaxy pair. In the north (south) survey field we find no evidence out to a redshift of greater than 0.5 (0.3) for cosmic strings to a mass per unit length limit of Gμ/c2<3.0×10-7 at 95% confidence limits (C.L.). In the combined 314.9  arcmin2 of the north and south survey fields this corresponds to a global limit on Ωstrings<0.02. Our limit on Gμ/c2 is more than an order of magnitude lower than searches for individual strings in cosmic microwave background (CMB) data. Our limit is higher than other CMB and gravitational wave searches, however, we note that it is less model dependent than these other searches.

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.77.123509
DOI:
10.1103/PhysRevD.77.123509
PACS:
98.80.Cq

*jlchrist@calpoly.edu