Blasi Simone, Brdar Vedran, Schmitz Kai
Max-Planck-Institut für Kernphysik, 69117 Heidelberg, Germany.
Theoretical Physics Department, CERN, 1211 Geneva 23, Switzerland.
Phys Rev Lett. 2021 Jan 29;126(4):041305. doi: 10.1103/PhysRevLett.126.041305.
The North American Nanohertz Observatory for Gravitational Waves has recently reported strong evidence for a stochastic common-spectrum process affecting the pulsar timing residuals in its 12.5-year data set. We demonstrate that this process admits an interpretation in terms of a stochastic gravitational-wave background emitted by a cosmic-string network in the early Universe. We study stable Nambu-Goto strings in dependence of their tension Gμ and loop size α and show that the entire viable parameter space will be probed by an array of future experiments.
北美纳赫兹引力波天文台最近报告了有力证据,表明存在一个随机共谱过程影响其12.5年数据集中的脉冲星计时残差。我们证明,这个过程可以解释为由早期宇宙中的宇宙弦网络发出的随机引力波背景。我们研究了稳定的南布-戈托弦与其张力Gμ和环大小α的关系,并表明未来一系列实验将探测整个可行的参数空间。