Broken blue-tilted inflationary gravitational waves: a joint analysis of NANOGrav 15-year and BICEP/Keck 2018 data

Broken blue-tilted inflationary gravitational waves: a joint analysis of NANOGrav 15-year and BICEP/Keck 2018 data
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DOI:
10.1088/1475-7516/2024/05/004
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发表时间:
2023-07
影响因子:
6.4
通讯作者:
Jun-Qian Jiang;Yong Cai;Gen Ye;Yun-song Piao
Jun-Qian Jiang;Yong Cai;Gen Ye;Yun-song Piao
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
Jun-Qian Jiang;Yong Cai;Gen Ye;Yun-song Piao

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最近,脉冲星计时阵列(PTA)合作报告了纳赫兹波段随机引力波背景(SGWB)的证据。暴胀引力波(IGW)的频谱是未知的,它在不同的频段可能呈现不同的幂律,因此如果PTA信号是原始的,那么利用当前的PTA和CMB数据研究IGW的潜在意义将是非常有意义的。在这封信中,我们使用NANOGrav 15年和BICEP/Keck 2018数据对IGW的破幂律谱进行了联合马尔可夫链蒙特卡罗分析。发现在PTA波段,IGW的最佳拟合谱倾斜为nPTA T = 2.42+0.32 - 0.91,而在CMB波段,最佳拟合谱倾斜为nCMB T = 0.55+0.37 - 0.10,而r的可探测幅度与nCMB T = 0.50仍是相容的。我们的结果的通货膨胀的影响进行了讨论。
Recently, the pulsar timing array (PTA) collaborations have reported the evidence for a stochastic gravitational wave background (SGWB) at nano-Hertz band. The spectrum of inflationary gravitational wave (IGW) is unknown, which might exhibit different power law at different frequency-bands, thus if the PTA signal is primordial, it will be significant to explore the underlying implications of current PTA and CMB data on IGW. In this Letter, we perform a joint Markov Chain Monte Carlo analysis for a broken power-law spectrum of IGW with the NANOGrav 15-year and BICEP/Keck 2018 data. It is found that though the bestfit spectral tilt of IGW at PTA band is n PTA T = 2.42+0.32 -0.91, at CMB band the bestfit is n CMB T = 0.55+0.37 -0.10 while a detectable amplitude of r with n CMB T ≃ 0 is still compatible. The implication of our results for inflation is also discussed.