| dc.contributor.author | Chakrabarty, Deepto | |
| dc.date.accessioned | 2020-06-08T20:07:02Z | |
| dc.date.available | 2020-06-08T20:07:02Z | |
| dc.date.issued | 2019-12 | |
| dc.identifier.issn | 2041-8213 | |
| dc.identifier.issn | 2041-8205 | |
| dc.identifier.uri | https://hdl.handle.net/1721.1/125720 | |
| dc.description.abstract | We describe the model of surface emission from a rapidly rotating neutron star that is applied to Neutron Star Interior Composition Explorer X-ray data of millisecond pulsars in order to statistically constrain the neutron star mass-radius relation and dense matter equation of state. To ensure that the associated calculations are both accurate and precise, we conduct an extensive suite of verification tests between our numerical codes for both the Schwarzschild + Doppler and Oblate Schwarzschild approximations, and compare both approximations against exact numerical calculations. We find superb agreement between the code outputs, as well as in comparisons against a set of analytical and semi-analytical calculations, which, combined with their speed, demonstrates that the codes are well suited for large-scale statistical sampling applications. A set of verified, high-precision reference synthetic pulse profiles is provided to the community to facilitate testing of other independently developed codes. | en_US |
| dc.language.iso | en | |
| dc.publisher | American Astronomical Society | en_US |
| dc.relation.isversionof | https://dx.doi.org/10.3847/2041-8213/ab5968 | en_US |
| dc.rights | Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. | en_US |
| dc.source | The American Astronomical Society | en_US |
| dc.title | Constraining the Neutron Star Mass-Radius Relation and Dense Matter Equation of State with NICER. II. Emission from Hot Spots on a Rapidly Rotating Neutron Star | en_US |
| dc.type | Article | en_US |
| dc.identifier.citation | Bogdanov, Slavko et al. “Constraining the Neutron Star Mass-Radius Relation and Dense Matter Equation of State with NICER. II. Emission from Hot Spots on a Rapidly Rotating Neutron Star” Astrophysical Journal Letters, vol. 887, no. 1, 2019, L26 © 2019 The Author(s) | en_US |
| dc.contributor.department | Massachusetts Institute of Technology. Department of Physics | en_US |
| dc.contributor.department | MIT Kavli Institute for Astrophysics and Space Research | en_US |
| dc.relation.journal | Astrophysical Journal Letters | en_US |
| dc.eprint.version | Final published version | en_US |
| dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
| eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
| dc.date.updated | 2020-03-30T15:04:44Z | |
| dspace.date.submission | 2020-03-30T15:04:46Z | |
| mit.journal.volume | 887 | en_US |
| mit.journal.issue | 1 | en_US |
| mit.license | PUBLISHER_POLICY | |
| mit.metadata.status | Complete | |
