Kasliwal, MM, Nakar, E, Singer, LP, Kaplan, DL, Cook, DO, Van Sistine, A, Lau, RM, Fremling, C, Gottlieb, O, Jencson, JE, Adams, SM, Feindt, U, Hotokezaka, K, Ghosh, S, Perley, DA, Yu, P-C, Piran, T, Allison, JR, Anupama, GC, Balasubramanian, A et al (2017) Illuminating gravitational waves: A concordant picture of photons from a neutron star merger. Science. ISSN 1095-9203
Full text not available from this repository. Please see publisher or open access link below:Abstract
Merging neutron stars offer an exquisite laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart (EM170817) to gravitational waves (GW170817) detected from merging neutron stars. By synthesizing a panchromatic dataset, we demonstrate that merging neutron stars are a long-sought production site forging heavy elements by r-process nucleosynthesis. The weak gamma-rays seen in EM170817 are dissimilar to classical short gamma-ray bursts with ultra-relativistic jets. Instead, we suggest that breakout of a wide-angle, mildly-relativistic cocoon engulfing the jet elegantly explains the low-luminosity gamma-rays, the high-luminosity ultraviolet-optical-infrared and the delayed radio/x-ray emission. We posit that all merging neutron stars may lead to a wide-angle cocoon breakout; sometimes accompanied by a successful jet and sometimes a choked jet.
Item Type: | Article |
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Uncontrolled Keywords: | MD Multidisciplinary |
Subjects: | Q Science > QB Astronomy Q Science > QC Physics Q Science > QD Chemistry |
Divisions: | Astrophysics Research Institute |
Publisher: | American Association for the Advancement of Science |
Related URLs: | |
Date of acceptance: | 5 October 2017 |
Date Deposited: | 31 Oct 2017 11:38 |
Last Modified: | 03 Sep 2021 23:33 |
DOI or ID number: | 10.1126/science.aap9455 |
URI: | https://ljmu-9.eprints-hosting.org/id/eprint/7446 |
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