تقرير
The NANOGrav 11 yr data set: Limits on Gravitational Wave Memory
| العنوان: | The NANOGrav 11 yr data set: Limits on Gravitational Wave Memory |
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| المؤلفون: | K Aggarwal, Zaven Arzoumanian, P T Baker, A Brazier, P R Brook, S Burke-Spolaor, S Chatterjee, J M Cordes, N J Cornish, F Crawford, H T Cromartie, K Crowter, M DeCesar, P B Demorest, T Dolch, J A Ellis, R D Ferdman, E C Ferrara, E Fonseca, N Garver-Daniels, P Gentile, M L Jones, D L Kaplan, L Z Kelley, J S Key, M T Lam, T J W Lazio, L Levin, D R Lorimer, J Luo, R S Lynch, D R Madison, M A McLaughlin, S T McWilliams, C M F Mingarelli, C Ng, D J Nice, T T Pennucci, N S Pol, S M Ransom, P S Ray, X Siemens, J Simon, R Spiewak, I H Stairs, D R Stinebring, K Stovall, J K Swiggum, S R Taylor, M Vallisneri, R van Haasteren, S J Vigeland, C A Witt, W W Zhu |
| المصدر: | Astrophysical Journal. 889(38) |
| بيانات النشر: | United States: NASA Center for Aerospace Information (CASI), 2020. |
| سنة النشر: | 2020 |
| مصطلحات موضوعية: | Astronomy |
| الوصف: | The mergers of supermassive black hole binaries (SMBHBs) promise to be incredible sources of gravitational waves (GWs).While the oscillatory part of the merger gravitational waveform will be outside the frequency sensitivity range of pulsar timing arrays, the nonoscillatory GW memory effect is detectable. Further, any burst of GWs will produce GW memory, making memory a useful probe of unmodeled exotic sources and new physics. We searched the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) 11 yr data set for GW memory. This data set is sensitive to very low-frequency GWs of ∼3 to 400 nHz (periods of ∼11 yr–1 month). Finding no evidence for GWs, we placed limits on the strain amplitude of GW memory events during the observation period. We then used the strain upper limits to place limits on the rate of GW memory causing events. At a strain of 2.5 × 10−14, corresponding to the median upper limit as a function of source sky position, we set a limit on the rate of GW memory events at <0.4 yr−1. That strain corresponds to an SMBHB merger with reduced mass of ηM ~2 × 1010Mmoonand inclination of ι = π/3 at a distance of 1 Gpc. As a test of our analysis, we analyzed the NANOGrav 9 yr data set as well. This analysis found an anomolous signal, which does not appear in the 11 yr data set. This signal is not a GW, and its origin remains unknown. |
| نوع الوثيقة: | Report |
| اللغة: | English |
| تدمد: | 1538-4357 0004-637X |
| DOI: | 10.3847/1538-4357/ab6083 |
| الوصول الحر: | https://ntrs.nasa.gov/citations/20210010596Test |
| ملاحظات: | 273493 80GSFC17M0002 |
| رقم الانضمام: | edsnas.20210010596 |
| قاعدة البيانات: | NASA Technical Reports |
Full Text Finder | تدمد: | 15384357 0004637X |
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| DOI: | 10.3847/1538-4357/ab6083 |