Estimating the EOS from the measurement of NS radii with 5% accuracy
Estimating the EOS from the measurement of NS radii with 5% accuracy
About this item
Full title
Author / Creator
Sieniawska, M , Bejger, M and Haskell, B
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
Formats
Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
Subjects
More information
Scope and Contents
Contents
Observations of heavy (\({\simeq}2\,M_\odot\)) neutron stars in addition to the recent measurement of tidal deformability from the binary neutron-star merger GW170817, place interesting constraints on theories of dense matter. Current and future observatories, such as the NICER and ATHENA are expected to collect information on the global parameters...
Alternative Titles
Full title
Estimating the EOS from the measurement of NS radii with 5% accuracy
Authors, Artists and Contributors
Author / Creator
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2073882600
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2073882600
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1803.08813
