Downloads provided by UsageCounts
doi: 10.3847/1538-4357/aaf21d , 10.18452/26483 , 10.48550/arxiv.1810.10693 , 10.3204/pubdb-2020-04065 , 10.25916/sut.26326333.v1 , 10.18154/rwth-2020-09814 , 10.25916/sut.26326333
arXiv: 1810.10693
handle: 10261/207170 , 10481/58798 , 2117/128069 , 10550/72555 , https://repository.ubn.ru.nl/handle/2066/201608 , 11588/739516 , 11368/3003384 , 11245.1/3e3989f1-c1e8-47dd-9f2c-d4aa02339bdd , 1871.1/c193b2f8-b264-400c-b6d3-ac3546be6947 , 2066/201608 , 10281/243087 , 2268/252440 , 11388/353790 , 21.11116/0000-0002-E7EE-E , 21.11116/0000-0002-6D6A-E , 21.11116/0000-0002-6D6C-C , 11572/231144 , 11576/2664163 , 11577/3286575 , 11386/4720687 , 2108/251020 , 11573/1263335 , 11584/410227 , 11581/447886 , 11567/938765 , 11568/952794 , 11591/464216 , 11585/658696 , 20.500.11769/599485 , 1854/LU-8620598 , 1959.3/447355 , 2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/297634 , 1885/205740 , 11381/2863333 , 2440/117851 , 1721.1/132135.2 , 1721.1/132135 , 1808/31013
doi: 10.3847/1538-4357/aaf21d , 10.18452/26483 , 10.48550/arxiv.1810.10693 , 10.3204/pubdb-2020-04065 , 10.25916/sut.26326333.v1 , 10.18154/rwth-2020-09814 , 10.25916/sut.26326333
arXiv: 1810.10693
handle: 10261/207170 , 10481/58798 , 2117/128069 , 10550/72555 , https://repository.ubn.ru.nl/handle/2066/201608 , 11588/739516 , 11368/3003384 , 11245.1/3e3989f1-c1e8-47dd-9f2c-d4aa02339bdd , 1871.1/c193b2f8-b264-400c-b6d3-ac3546be6947 , 2066/201608 , 10281/243087 , 2268/252440 , 11388/353790 , 21.11116/0000-0002-E7EE-E , 21.11116/0000-0002-6D6A-E , 21.11116/0000-0002-6D6C-C , 11572/231144 , 11576/2664163 , 11577/3286575 , 11386/4720687 , 2108/251020 , 11573/1263335 , 11584/410227 , 11581/447886 , 11567/938765 , 11568/952794 , 11591/464216 , 11585/658696 , 20.500.11769/599485 , 1854/LU-8620598 , 1959.3/447355 , 2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/297634 , 1885/205740 , 11381/2863333 , 2440/117851 , 1721.1/132135.2 , 1721.1/132135 , 1808/31013
Abstract Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.
Astrofísica, EVENTS GW150914, Gravitació, neutron star: binary, Aérospatiale, astronomie & astrophysique, neutrino: energy: high, Astronomy, RAY, ddc:520, Astronomical Sciences, Astrophysics, Astrophysics / csillagászat, Atomic, IceCube, Particle and Plasma Physics, Astronomi, astrofysik och kosmologi, black hole, QB Astronomy, Astronomy, Astrophysics and Cosmology, LIGO, ELECTROMAGNETIC SIGNALS, gravitational wave, QC, gravitational waves – neutrinos, QB, astro-ph.HE, 0306 Physical Chemistry (incl. Structural), High Energy Astrophysical Phenomena (astro-ph.HE), Physics, ddc:530, Space sciences, gravitational waves; neutrinos;, neutrinos, Particle and High Energy Physics, gravitational waves; neutrinos, 520 Astronomie und zugeordnete Wissenschaften, Nuclear and Plasma Physics, 520, Settore FIS/01 - FISICA SPERIMENTALE, QB460-466, observatory, gravitational waves, Particle and high energy physics, astrophysics: density, Physical Sciences, 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics, Astrophysics - High Energy Astrophysical Phenomena, info:eu-repo/classification/ddc/520, gravitational waves; neutrinos; Astronomy and Astrophysics; Space and Planetary Science, Astronomical and Space Sciences, 5101 Astronomical sciences, signature, Physical Chemistry (incl. Structural), Physique, chimie, mathématiques & sciences de la terre, supernova: collapse, FOS: Physical sciences, Astronomy & Astrophysics, 530, 5109 Space sciences, Gravitational waves, Physical, chemical, mathematical & earth Sciences, 5107 Particle and high energy physics, Ones gravitacionals, 0201 Astronomical and Space Sciences, Gravitational Waves, Neutrinos, LIGO, Virgo, Antares, IceCube, Nuclear, Àrees temàtiques de la UPC::Física::Astronomia i astrofísica, Neutrins, Neutrinos, STFC, Astrophysique, Science & Technology, ANTARES, Molecular, RCUK, Astronomy and Astrophysics, Astronomie, 530 Physik, Sciences de l'espace, messenger, asztrofizika, Physics and Astronomy, Space and Planetary Science, :Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], FISICA APLICADA, gravitational radiation: emission, Astronomical sciences, Space science, astronomy & astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], EMISSION, ddc: ddc:
Astrofísica, EVENTS GW150914, Gravitació, neutron star: binary, Aérospatiale, astronomie & astrophysique, neutrino: energy: high, Astronomy, RAY, ddc:520, Astronomical Sciences, Astrophysics, Astrophysics / csillagászat, Atomic, IceCube, Particle and Plasma Physics, Astronomi, astrofysik och kosmologi, black hole, QB Astronomy, Astronomy, Astrophysics and Cosmology, LIGO, ELECTROMAGNETIC SIGNALS, gravitational wave, QC, gravitational waves – neutrinos, QB, astro-ph.HE, 0306 Physical Chemistry (incl. Structural), High Energy Astrophysical Phenomena (astro-ph.HE), Physics, ddc:530, Space sciences, gravitational waves; neutrinos;, neutrinos, Particle and High Energy Physics, gravitational waves; neutrinos, 520 Astronomie und zugeordnete Wissenschaften, Nuclear and Plasma Physics, 520, Settore FIS/01 - FISICA SPERIMENTALE, QB460-466, observatory, gravitational waves, Particle and high energy physics, astrophysics: density, Physical Sciences, 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics, Astrophysics - High Energy Astrophysical Phenomena, info:eu-repo/classification/ddc/520, gravitational waves; neutrinos; Astronomy and Astrophysics; Space and Planetary Science, Astronomical and Space Sciences, 5101 Astronomical sciences, signature, Physical Chemistry (incl. Structural), Physique, chimie, mathématiques & sciences de la terre, supernova: collapse, FOS: Physical sciences, Astronomy & Astrophysics, 530, 5109 Space sciences, Gravitational waves, Physical, chemical, mathematical & earth Sciences, 5107 Particle and high energy physics, Ones gravitacionals, 0201 Astronomical and Space Sciences, Gravitational Waves, Neutrinos, LIGO, Virgo, Antares, IceCube, Nuclear, Àrees temàtiques de la UPC::Física::Astronomia i astrofísica, Neutrins, Neutrinos, STFC, Astrophysique, Science & Technology, ANTARES, Molecular, RCUK, Astronomy and Astrophysics, Astronomie, 530 Physik, Sciences de l'espace, messenger, asztrofizika, Physics and Astronomy, Space and Planetary Science, :Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], FISICA APLICADA, gravitational radiation: emission, Astronomical sciences, Space science, astronomy & astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], EMISSION, ddc: ddc:
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 37 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Top 10% | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Top 10% | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Top 10% |
| views | 228 | |
| downloads | 220 |

Views provided by UsageCounts
Downloads provided by UsageCounts