Gravitational-wave stochastic background from kinks and cusps on cosmic strings
We compute the contribution of kinks on cosmic string loops to stochastic background of gravitational waves (SBGW). We find that kinks contribute at the same order as cusps to the SBGW. We discuss the accessibility of the total background due to kinks as well as cusps to current and planned gravitat...
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Veröffentlicht in: | Physical review. D, Particles and fields Particles and fields, 2010-05, Vol.81 (10), Article 104028 |
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container_title | Physical review. D, Particles and fields |
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creator | Ölmez, S. Mandic, V. Siemens, X. |
description | We compute the contribution of kinks on cosmic string loops to stochastic background of gravitational waves (SBGW). We find that kinks contribute at the same order as cusps to the SBGW. We discuss the accessibility of the total background due to kinks as well as cusps to current and planned gravitational-wave detectors, as well as to the big bang nucleosynthesis (BBN), the cosmic microwave background (CMB), and pulsar timing constraints. As in the case of cusps, we find that current data from interferometric gravitational-wave detectors, such as LIGO, are sensitive to areas of parameter space of cosmic string models complementary to those accessible to pulsar, BBN, and CMB bounds. |
doi_str_mv | 10.1103/PhysRevD.81.104028 |
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D, Particles and fields</title><description>We compute the contribution of kinks on cosmic string loops to stochastic background of gravitational waves (SBGW). We find that kinks contribute at the same order as cusps to the SBGW. We discuss the accessibility of the total background due to kinks as well as cusps to current and planned gravitational-wave detectors, as well as to the big bang nucleosynthesis (BBN), the cosmic microwave background (CMB), and pulsar timing constraints. 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D, Particles and fields</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ölmez, S.</au><au>Mandic, V.</au><au>Siemens, X.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Gravitational-wave stochastic background from kinks and cusps on cosmic strings</atitle><jtitle>Physical review. D, Particles and fields</jtitle><date>2010-05-15</date><risdate>2010</risdate><volume>81</volume><issue>10</issue><artnum>104028</artnum><issn>1550-7998</issn><issn>0556-2821</issn><eissn>1550-2368</eissn><eissn>1089-4918</eissn><abstract>We compute the contribution of kinks on cosmic string loops to stochastic background of gravitational waves (SBGW). We find that kinks contribute at the same order as cusps to the SBGW. We discuss the accessibility of the total background due to kinks as well as cusps to current and planned gravitational-wave detectors, as well as to the big bang nucleosynthesis (BBN), the cosmic microwave background (CMB), and pulsar timing constraints. As in the case of cusps, we find that current data from interferometric gravitational-wave detectors, such as LIGO, are sensitive to areas of parameter space of cosmic string models complementary to those accessible to pulsar, BBN, and CMB bounds.</abstract><cop>United States</cop><doi>10.1103/PhysRevD.81.104028</doi></addata></record> |
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source | American Physical Society Journals |
subjects | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY COMPOSITE MODELS COMPUTERIZED SIMULATION COSMIC RADIO SOURCES CUSPED GEOMETRIES ELECTROMAGNETIC RADIATION EXTENDED PARTICLE MODEL GRAVITATIONAL WAVE DETECTORS GRAVITATIONAL WAVES MAGNETIC FIELD CONFIGURATIONS MATHEMATICAL MODELS MEASURING INSTRUMENTS MICROWAVE RADIATION NUCLEOSYNTHESIS OPEN CONFIGURATIONS PARTICLE MODELS PULSARS QUARK MODEL RADIATION DETECTORS RADIATIONS RELICT RADIATION SIMULATION SPACE STOCHASTIC PROCESSES STRING MODELS SYNTHESIS |
title | Gravitational-wave stochastic background from kinks and cusps on cosmic strings |
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