Direct determination of cosmic string loop density from simulations
Dec 20, 20195 pages
Published in:
- Phys.Rev.D 101 (2020) 10, 103018
- Published: May 15, 2020
e-Print:
- 1912.10017 [astro-ph.CO]
View in:
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Abstract: (APS)
We determine the distribution of cosmic string loops directly from simulations, rather than determining the loop production function and inferring the loop distribution from that. For a wide range of loop lengths, the results agree well with a power law exponent -2.5 in the radiation era and -2 in the matter era, the universal result for any loop production function that does not diverge at small scales. Our results extend those of Ringeval et al. [Cosmological evolution of cosmic string loops, J. Cosmol. Astropart. Phys. 02 (2007) 023.10.1088/1475-7516/2007/02/023]: we are able to run for 15 times longer in conformal time and simulate a volume 300–2400 times larger. At the times they reached, our simulation is in general agreement with the more negative exponents they found, -2.6 and -2.4. However, our simulations show that this was a transient regime; at later times, the exponents decline to the values above. This provides further evidence against models with a rapid divergence of the loop density at small scales, such as “model 3” used to analyze LIGO data and predict LISA sensitivity.Note:
- 10 pages, 3 figures
- Astrophysics and astroparticle physics
- time: conformal
- LISA: sensitivity
- cosmic string
- density
- LIGO
- numerical calculations
- numerical methods
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Figures(3)
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