摘要
Merging neutron stars offer an excellent laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart (EM170817) with gravitational waves (GW170817) detected from merging neutron stars. By synthesizing a panchromatic data set, 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 ultrarelativistic jets. Instead, we suggest that breakout of a wide-angle, mildly relativistic cocoon engulfing the jet explains the low-luminosity gamma rays, the high-luminosity ultraviolet-optical-infrared, and the delayed radio and x-ray emission. We posit that all neutron star mergers may lead to a wide-angle cocoon breakout, sometimes accompanied by a successful jet and sometimes by a choked jet.
| 原文 | ???core.languages.en_GB??? |
|---|---|
| 頁（從 - 到） | 1559-1565 |
| 頁數 | 7 |
| 期刊 | Science |
| 卷 | 358 |
| 發行號 | 6370 |
| DOIs | |
| 出版狀態 | 已出版 - 22 12月 2017 |
指紋
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於: Science, 卷 358, 編號 6370, 22.12.2017, p. 1559-1565.
研究成果: 雜誌貢獻 › 期刊論文 › 同行評審
TY - JOUR
T1 - Illuminating gravitational waves
T2 - A concordant picture of photons from a neutron star merger
AU - Kasliwal, M. M.
AU - Nakar, E.
AU - Singer, L. P.
AU - Kaplan, D. L.
AU - Cook, D. O.
AU - Van Sistine, A.
AU - Lau, R. M.
AU - Fremling, C.
AU - Gottlieb, O.
AU - Jencson, J. E.
AU - Adams, S. M.
AU - Feindt, U.
AU - Hotokezaka, K.
AU - Ghosh, S.
AU - Perley, D. A.
AU - Yu, P. C.
AU - Piran, T.
AU - Allison, J. R.
AU - Anupama, G. C.
AU - Balasubramanian, A.
AU - Bannister, K. W.
AU - Bally, J.
AU - Barnes, J.
AU - Barway, S.
AU - Bellm, E.
AU - Bhalerao, V.
AU - Bhattacharya, D.
AU - Blagorodnova, N.
AU - Bloom, J. S.
AU - Brady, P. R.
AU - Cannella, C.
AU - Chatterjee, D.
AU - Cenko, S. B.
AU - Cobb, B. E.
AU - Copperwheat, C.
AU - Corsi, A.
AU - De, K.
AU - Dobie, D.
AU - Emery, S. W.K.
AU - Evans, P. A.
AU - Fox, O. D.
AU - Frail, D. A.
AU - Frohmaier, C.
AU - Goobar, A.
AU - Hallinan, G.
AU - Harrison, F.
AU - Helou, G.
AU - Hinderer, T.
AU - Ho, A. Y.Q.
AU - Horesh, A.
AU - Ip, W. H.
AU - Itoh, R.
AU - Kasen, D.
AU - Kim, H.
AU - Kuin, N. P.M.
AU - Kupfer, T.
AU - Lynch, C.
AU - Madsen, K.
AU - Mazzali, P. A.
AU - Miller, A. A.
AU - Mooley, K.
AU - Murphy, T.
AU - Ngeow, C. C.
AU - Nichols, D.
AU - Nissanke, S.
AU - Nugent, P.
AU - Ofek, E. O.
AU - Qi, H.
AU - Quimby, R. M.
AU - Rosswog, S.
AU - Rusu, F.
AU - Sadler, E. M.
AU - Schmidt, P.
AU - Sollerman, J.
AU - Steele, I.
AU - Williamson, A. R.
AU - Xu, Y.
AU - Yan, L.
AU - Yatsu, Y.
AU - Zhang, C.
AU - Zhao, W.
N1 - Funding Information: We thank I. Kostadinova for seamlessly coordinating the GROWTH (Global Relay of Observatories Watching Transients Happen) project; B. Griswold for beautiful graphic art; P. Whitelock for facilitating InfraRed Survey Facility observations; S. Barthelmy for setting up a Ligo Virgo Consortium Gamma-ray Coordination Network system that facilitated quick, citable communication between astronomers and maximized the science return; S. Phinney, S. Kulkarni, and L. Bildsten for valuable comments; the staff of Gemini Observatory, particularly the director, L. Ferrarese, for rapidly approving our Director’s Discretionary Time request; and our program contact scientists M. Shirmer, H. Kim, K. Silva, M. Andersen, and R. Salinas for supporting and executing observations. We are especially grateful to Gemini for postponing scheduled maintenance on the FLAMINGOS-2 instrument to allow us to obtain as much data as possible on this extraordinary event. This work was supported by the GROWTH project funded by the National Science Foundation under Partnerships for International Research and Education grant no. 1545949. GROWTH is a collaborative project among the California Institute of Technology (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Texas Tech University (USA), San Diego State University (USA), Los Alamos National Laboratory (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Inter-University Center for Astronomy and Astrophysics (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany), and Liverpool John Moores University (UK). Full facility and funding acknowledgements are provided in the supplementary materials. The photometric data that we used are tabulated in table S1. All of our raw observations are available in observatory archives; URLs and project numbers are provided in the supplementary materials. The PLUTO software used for our simulations is available at http://plutocode.ph.unito.it/; our simulation input and output files are provided as data S1 and S2. Funding Information: We thank I. Kostadinova for seamlessly coordinating the GROWTH (Global Relay of Observatories Watching Transients Happen) project; B. Griswold for beautiful graphic art; P. Whitelock for facilitating InfraRed Survey Facility observations; S. Barthelmy for setting up a Ligo Virgo Consortium Gamma-ray Coordination Network system that facilitated quick, citable communication between astronomers and maximized the science return; S. Phinney, S. Kulkarni, and L. Bildsten for valuable comments; the staff of Gemini Observatory, particularly the director, L. Ferrarese, for rapidly approving our Director?s Discretionary Time request; and our program contact scientists M. Shirmer, H. Kim, K. Silva, M. Andersen, and R. Salinas for supporting and executing observations. We are especially grateful to Gemini for postponing scheduled maintenance on the FLAMINGOS-2 instrument to allow us to obtain as much data as possible on this extraordinary event. This work was supported by the GROWTH project funded by the National Science Foundation under Partnerships for International Research and Education grant no. 1545949. GROWTH is a collaborative project among the California Institute of Technology (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Texas Tech University (USA), San Diego State University (USA), Los Alamos National Laboratory (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Inter-University Center for Astronomy and Astrophysics (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany), and Liverpool John Moores University (UK). Full facility and funding acknowledgements are provided in the supplementary materials. The photometric data that we used are tabulated in table S1. All of our raw observations are available in observatory archives; URLs and project numbers are provided in the supplementary materials. The PLUTO software used for our simulations is available at http://plutocode.ph.unito.it/; our simulation input and output files are provided as data S1 and S2.
PY - 2017/12/22
Y1 - 2017/12/22
N2 - Merging neutron stars offer an excellent laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart (EM170817) with gravitational waves (GW170817) detected from merging neutron stars. By synthesizing a panchromatic data set, 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 ultrarelativistic jets. Instead, we suggest that breakout of a wide-angle, mildly relativistic cocoon engulfing the jet explains the low-luminosity gamma rays, the high-luminosity ultraviolet-optical-infrared, and the delayed radio and x-ray emission. We posit that all neutron star mergers may lead to a wide-angle cocoon breakout, sometimes accompanied by a successful jet and sometimes by a choked jet.
AB - Merging neutron stars offer an excellent laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart (EM170817) with gravitational waves (GW170817) detected from merging neutron stars. By synthesizing a panchromatic data set, 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 ultrarelativistic jets. Instead, we suggest that breakout of a wide-angle, mildly relativistic cocoon engulfing the jet explains the low-luminosity gamma rays, the high-luminosity ultraviolet-optical-infrared, and the delayed radio and x-ray emission. We posit that all neutron star mergers may lead to a wide-angle cocoon breakout, sometimes accompanied by a successful jet and sometimes by a choked jet.
UR - http://www.scopus.com/inward/record.url?scp=85031781920&partnerID=8YFLogxK
U2 - 10.1126/science.aap9455
DO - 10.1126/science.aap9455
M3 - 期刊論文
C2 - 29038373
AN - SCOPUS:85031781920
SN - 0036-8075
VL - 358
SP - 1559
EP - 1565
JO - Science
JF - Science
IS - 6370
ER -