Powered by OpenAIRE graph
Found an issue? Give us feedback
ZENODOarrow_drop_down
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2024
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2024
License: CC BY
Data sources: Datacite
versions View all 6 versions
addClaim

This Research product is the result of merged Research products in OpenAIRE.

You have already added 0 works in your ORCID record related to the merged Research product.

Data table for EoS SFH(SFHo) neutron matter (no electrons) nparam=2

Authors: Chatterjee, Debarati; Davis, Philip; Dexheimer, Veronica; Ishizuka, Chikako; Klähn, Thomas; Mancini, Marco; Oertel, Micaela; +7 Authors

Data table for EoS SFH(SFHo) neutron matter (no electrons) nparam=2

Abstract

The data table for the EoS SFH(SFHo) neutron matter (no electrons) of the family Neutron Matter EoS with 2 parameters can be found via this link compose.obspm.fr/eos/13 together with additional information on the EoS. Please be aware that in particular the authors of the equation of state can be found in the references below and on the Compose data base ( compose.obspm.fr/eos/13). Thus if you use this entry, please cite the original references together with the link to the table. We are working currently on rectifying the automatic citation from zenodo with author information on the equation of state. The online service CompOSE provides data tables for different state of the art equations of state (EoS) ready for further usage in astrophysical applications, nuclear physics and beyond. CompOSE would not be possible without the financial and organizational support from a large number of institutions and individual contributors. In particular, we gratefully acknowledge support by : CompStar, Research Networking Programs of the European Science Foundation (ESF) NewCompStar, "Exploring fundamental physics with compact stars" (MPNS COST action MP1304). PHAROS, "The multi-messenger physics and astrophysics of neutron stars" within the EU framework programme (COST action CA16214).

Keywords

A stars, Neutron star cores, Core-collapse supernovae, Nuclear physics, Nuclear astrophysics, Compact objects, Neutron stars

  • BIP!
    Impact byBIP!
    citations
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    0
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    Average
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    Average
Powered by OpenAIRE graph
Found an issue? Give us feedback
citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average