Gravitational-wave detections are enabling measurements of the rate of coalescences of binaries composed of two compact objects—neutron stars and/or black holes. The …
BP Abbott, R Abbott, TD Abbott, S Abraham… - Physical Review X, 2019 - APS
We present the results from three gravitational-wave searches for coalescing compact binaries with component masses above 1 M⊙ during the first and second observing runs of …
D Kasen, B Metzger, J Barnes, E Quataert… - Nature, 2017 - nature.com
The cosmic origin of elements heavier than iron has long been uncertain. Theoretical modelling,,,,,, shows that the matter that is expelled in the violent merger of two neutron stars …
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley… - Physical review …, 2017 - APS
On August 17, 2017 at 12∶ 41: 04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral …
On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
JP Naiman, A Pillepich, V Springel… - Monthly Notices of …, 2018 - academic.oup.com
The distribution of elements in galaxies provides a wealth of information about their production sites and their subsequent mixing into the interstellar medium. Here we …
Double neutron star (DNS) systems represent extreme physical objects and the endpoint of an exotic journey of stellar evolution and binary interactions. Large numbers of DNS systems …
BS Acharya, I Agudo, I Al Samarai, R Alfaro, J Alfaro… - 2019 - air.uniud.it
Names: CTA Consortium (Organization) Title: Science with the Cherenkov Telescope Array/by The CTA Consortium. Description: New Jersey: World Scientific, 2018.| Includes …