New method to observe gravitational waves emitted by core collapse supernovae-Reference-Cited by-同舟云学术

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New method to observe gravitational waves emitted by core collapse supernovae

Published:2018-12-10 Issue:12 Volume:98 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Astone P.,Cerdá-Durán P.,Di Palma I.,Drago M.,Muciaccia F.,Palomba C.,Ricci F.

Funder

Sapienza Università di Roma

Ministerio de Economía y Competitividad

Generalitat Valenciana

Istituto Nazionale di Fisica Nucleare of Italy

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.98.122002/fulltext

Reference48 articles.

1. Observation of Gravitational Waves from a Binary Black Hole Merger

2. GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

3. GW170608: Observation of a 19 Solar-mass Binary Black Hole Coalescence

4. GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence

5. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

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1. Deep-learning classification and parameter inference of rotational core-collapse supernovae;Physical Review D;2024-09-11

2. The gravitational-wave emission from the explosion of a 15 solar mass star with rotation and magnetic fields;Monthly Notices of the Royal Astronomical Society;2024-07-23

3. Detection of Gravitational Waves Using Machine Learning;2024 5th International Conference for Emerging Technology (INCET);2024-05-24

4. Visualizing convolutional neural network for classifying gravitational waves from core-collapse supernovae;Physical Review D;2023-12-20

5. Multimessenger observations of core-collapse supernovae: Exploiting the standing accretion shock instability;Physical Review D;2023-11-22

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