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Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang t...

Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang t...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3128430763

Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform

About this item

Full title

Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2024-11

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Core-collapse supernovae (CCSNe) are potential multimessenger events detectable by current and future gravitational wave (GW) detectors. The GW signals emitted during these events are expected to provide insights into the explosion mechanism and the internal structures of neutron stars. In recent years, several studies have empirically derived the...

Alternative Titles

Full title

Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_3128430763

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3128430763

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2411.08407

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