English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Nuclear reactions may affect gravitational-wave signals from neutron-starmergers, but the impact is uncertain. In order to quantify the effect, wecompare two numerical simulations representing intuitive extremes. In one casereactions happen instantaneously. In the other case, they occur on timescalesmuch slower than the evolutionary timescale. We show that, while thedifferences in the two gravitational-wave signals are small, they should bedetectable by third-generation observatories. To avoid systematic errors inequation of state parameters inferred from observed signals, we need toaccurately implement nuclear reactions in future simulations.

Detecting the impact of nuclear reactions on neutron star mergers through gravitational waves