scholarly journals Arc minute gravitational lenses and cosmic strings

Nature ◽  
1986 ◽  
Vol 324 (6095) ◽  
pp. 392-392
Author(s):  
DAVID P. BENNETT ◽  
ALBERT STEBBINS
Nature ◽  
1986 ◽  
Vol 324 (6095) ◽  
pp. 392-393 ◽  
Author(s):  
P. PACZYŃSKI

1984 ◽  
Vol 282 ◽  
pp. L51 ◽  
Author(s):  
A. Vilenkin

1988 ◽  
Vol 130 ◽  
pp. 600-600
Author(s):  
Rachel Webster ◽  
Paul Hewett

Cosmic strings would be cosmologically interesting if they acted as seeds for rich cluster and galaxy formation. Most comological scenarios require the mean mass density per unit length of the string μ to be ∼ 2 × 10−6 for cosmic strings to act as seeds. If there is a population of long-lived cosmic strings which are either long loops or infinite strings, then they will gravit ationally lense background sources (Vilenkin 1984). We are undertaking a substantial survey for multiply imaged optical quasars. So far we have examined ∼ 2500 quasars and have no candidate multiply imaged quasars with separations ≳ 13″ (Webster et aJ. 1987). This sample will double over the next year. The survey will detect multiply imaged quasars with the image separations predicted if one has a population of cosmic strings with μ ∼ 2 × 10−6 acting as gravitational lenses. In due course, this survey will enable us to confirm or rule out the possibility that cosmic strings seed galaxy formation.


1999 ◽  
Vol 117 (5) ◽  
pp. 2034-2038 ◽  
Author(s):  
John L. Tonry ◽  
Christopher S. Kochanek
Keyword(s):  

Nature ◽  
2017 ◽  
Vol 548 (7669) ◽  
pp. 555-557 ◽  
Author(s):  
Yashar D. Hezaveh ◽  
Laurence Perreault Levasseur ◽  
Philip J. Marshall

2021 ◽  
Vol 2021 (5) ◽  
Author(s):  
Klaas Parmentier

Abstract We demonstrate that all rigidly rotating strings with center of mass at the origin of the dS3 static patch satisfy the Higuchi bound. This extends the observation of Noumi et al. for the open GKP-like string to all solutions of the Larsen-Sanchez class. We argue that strings violating the bound end up expanding towards the horizon and provide a numerical example. Adding point masses to the open string only increases the mass/spin ratio. For segmented strings, we write the conserved quantities, invariant under Gubser’s algebraic evolution equation, in terms of discrete lightcone coordinates describing kink collisions. Randomly generated strings are found to have a tendency to escape through the horizon that is mostly determined by their energy. For rapidly rotating segmented strings with mass/spin < 1, the kink collisions eventually become causally disconnected. Finally we consider the scenario of cosmic strings captured by a black hole in dS and find that horizon friction can make the strings longer.


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