Abstract
Motivated by the recent claim for gravitational lensing by a cosmic string, we reinvestigate the probability of finding such an event with upcoming wide-field surveys. If an observed lensing event is suspected to be due to a string, observations of the vicinity of the event in a circle of diameter L centered on the observed lens should reveal several additional lensing events. For a string located nearby (z≤0.5), we find that observations in a region of size ≈ 1 arc min2 will see ∼100 objects, of which ∼5 would be lensed by the string, compared to ∼0.1 lensed by conventional sources.
| Original language | English (US) |
|---|---|
| Article number | 041301 |
| Journal | Physical Review D |
| Volume | 68 |
| Issue number | 4 |
| DOIs | |
| State | Published - 2003 |
| Externally published | Yes |
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ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)
- Physics and Astronomy(all)
- Nuclear and High Energy Physics
- Mathematical Physics
Cite this
Gravitational lensing by cosmic strings in the era of wide-field surveys. / Huterer, Dragan; Vachaspati, Tanmay.
In: Physical Review D, Vol. 68, No. 4, 041301, 2003.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Gravitational lensing by cosmic strings in the era of wide-field surveys
AU - Huterer, Dragan
AU - Vachaspati, Tanmay
PY - 2003
Y1 - 2003
N2 - Motivated by the recent claim for gravitational lensing by a cosmic string, we reinvestigate the probability of finding such an event with upcoming wide-field surveys. If an observed lensing event is suspected to be due to a string, observations of the vicinity of the event in a circle of diameter L centered on the observed lens should reveal several additional lensing events. For a string located nearby (z≤0.5), we find that observations in a region of size ≈ 1 arc min2 will see ∼100 objects, of which ∼5 would be lensed by the string, compared to ∼0.1 lensed by conventional sources.
AB - Motivated by the recent claim for gravitational lensing by a cosmic string, we reinvestigate the probability of finding such an event with upcoming wide-field surveys. If an observed lensing event is suspected to be due to a string, observations of the vicinity of the event in a circle of diameter L centered on the observed lens should reveal several additional lensing events. For a string located nearby (z≤0.5), we find that observations in a region of size ≈ 1 arc min2 will see ∼100 objects, of which ∼5 would be lensed by the string, compared to ∼0.1 lensed by conventional sources.
UR - http://www.scopus.com/inward/record.url?scp=0141433453&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0141433453&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.68.041301
DO - 10.1103/PhysRevD.68.041301
M3 - Article
AN - SCOPUS:0141433453
VL - 68
JO - Physical review D: Particles and fields
JF - Physical review D: Particles and fields
SN - 1550-7998
IS - 4
M1 - 041301
ER -