Properties and Dynamics of Neutron Stars and Proto-Neutron Stars
Following new developments in the measurement of gravitational waves from neutron–star mergers and the modification or construction of particle colliders to reach larger densities, we are entering a new era, during which we can begin to understand dense and hot matter for the first time. This, toge...
Saved in:
HerausgeberIn: | |
---|---|
Sonstige: | |
Year of Publication: | 2022 |
Language: | English |
Physical Description: | 1 electronic resource (252 p.) |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
id |
993562961804498 |
---|---|
ctrlnum |
(CKB)5670000000391648 (oapen)https://directory.doabooks.org/handle/20.500.12854/93270 (EXLCZ)995670000000391648 |
collection |
bib_alma |
record_format |
marc |
spelling |
Dexheimer, Veronica edt Properties and Dynamics of Neutron Stars and Proto-Neutron Stars MDPI - Multidisciplinary Digital Publishing Institute 2022 1 electronic resource (252 p.) text txt rdacontent computer c rdamedia online resource cr rdacarrier Following new developments in the measurement of gravitational waves from neutron–star mergers and the modification or construction of particle colliders to reach larger densities, we are entering a new era, during which we can begin to understand dense and hot matter for the first time. This, together with future supernova explosion data, will provide us with the opportunity to have truly multimessenger data on hot and dense matter, which is, to some extent, similar to the matter present in the core of proto-neutron stars. This Special Issue focuses on the theory necessary to understand present and future data. It includes state-of-the-art theoretical models that describe dense and hot matter and dynamical stellar simulations that make use of them, with the ultimate goal of determining which degrees of freedom are relevant under these conditions and how they affect the matter equation of state and stellar evolution. English Research & information: general bicssc Physics bicssc neutron stars equations of state relativistic models gravitational waves neutron star equation of state universal relation hybrid star color superconductivity diquark dense matter neutrinos hyperons nuclear matter neutron star merger beta equilibration weak interaction chiral symmetry axion QED quark-hole pairing cold-dense QCD magnetic DCDW quark stars dark matter radial oscillations nuclear matter aspects quark deconfinement quark-gluon plasma production phase-transition neutron star crust meson interactions quantum molecular dynamics 3-0365-5399-1 Negreiros, Rodrigo edt Dexheimer, Veronica oth Negreiros, Rodrigo oth |
language |
English |
format |
eBook |
author2 |
Negreiros, Rodrigo Dexheimer, Veronica Negreiros, Rodrigo |
author_facet |
Negreiros, Rodrigo Dexheimer, Veronica Negreiros, Rodrigo |
author2_variant |
v d vd r n rn |
author2_role |
HerausgeberIn Sonstige Sonstige |
title |
Properties and Dynamics of Neutron Stars and Proto-Neutron Stars |
spellingShingle |
Properties and Dynamics of Neutron Stars and Proto-Neutron Stars |
title_full |
Properties and Dynamics of Neutron Stars and Proto-Neutron Stars |
title_fullStr |
Properties and Dynamics of Neutron Stars and Proto-Neutron Stars |
title_full_unstemmed |
Properties and Dynamics of Neutron Stars and Proto-Neutron Stars |
title_auth |
Properties and Dynamics of Neutron Stars and Proto-Neutron Stars |
title_new |
Properties and Dynamics of Neutron Stars and Proto-Neutron Stars |
title_sort |
properties and dynamics of neutron stars and proto-neutron stars |
publisher |
MDPI - Multidisciplinary Digital Publishing Institute |
publishDate |
2022 |
physical |
1 electronic resource (252 p.) |
isbn |
3-0365-5400-9 3-0365-5399-1 |
illustrated |
Not Illustrated |
work_keys_str_mv |
AT dexheimerveronica propertiesanddynamicsofneutronstarsandprotoneutronstars AT negreirosrodrigo propertiesanddynamicsofneutronstarsandprotoneutronstars |
status_str |
n |
ids_txt_mv |
(CKB)5670000000391648 (oapen)https://directory.doabooks.org/handle/20.500.12854/93270 (EXLCZ)995670000000391648 |
carrierType_str_mv |
cr |
is_hierarchy_title |
Properties and Dynamics of Neutron Stars and Proto-Neutron Stars |
author2_original_writing_str_mv |
noLinkedField noLinkedField noLinkedField |
_version_ |
1796652159187550208 |
fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>03028nam-a2200709z--4500</leader><controlfield tag="001">993562961804498</controlfield><controlfield tag="005">20231214133031.0</controlfield><controlfield tag="006">m o d </controlfield><controlfield tag="007">cr|mn|---annan</controlfield><controlfield tag="008">202210s2022 xx |||||o ||| 0|eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">3-0365-5400-9</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(CKB)5670000000391648</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(oapen)https://directory.doabooks.org/handle/20.500.12854/93270</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(EXLCZ)995670000000391648</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Dexheimer, Veronica</subfield><subfield code="4">edt</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Properties and Dynamics of Neutron Stars and Proto-Neutron Stars</subfield></datafield><datafield tag="260" ind1=" " ind2=" "><subfield code="b">MDPI - Multidisciplinary Digital Publishing Institute</subfield><subfield code="c">2022</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 electronic resource (252 p.)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">computer</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">online resource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Following new developments in the measurement of gravitational waves from neutron–star mergers and the modification or construction of particle colliders to reach larger densities, we are entering a new era, during which we can begin to understand dense and hot matter for the first time. This, together with future supernova explosion data, will provide us with the opportunity to have truly multimessenger data on hot and dense matter, which is, to some extent, similar to the matter present in the core of proto-neutron stars. This Special Issue focuses on the theory necessary to understand present and future data. It includes state-of-the-art theoretical models that describe dense and hot matter and dynamical stellar simulations that make use of them, with the ultimate goal of determining which degrees of freedom are relevant under these conditions and how they affect the matter equation of state and stellar evolution.</subfield></datafield><datafield tag="546" ind1=" " ind2=" "><subfield code="a">English</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Research & information: general</subfield><subfield code="2">bicssc</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Physics</subfield><subfield code="2">bicssc</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">neutron stars</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">equations of state</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">relativistic models</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">gravitational waves</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">neutron star</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">equation of state</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">universal relation</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">hybrid star</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">color superconductivity</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">diquark</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">dense matter</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">neutrinos</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">hyperons</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">nuclear matter</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">neutron star merger</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">beta equilibration</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">weak interaction</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">chiral symmetry</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">axion QED</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">quark-hole pairing</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">cold-dense QCD</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">magnetic DCDW</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">quark stars</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">dark matter</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">radial oscillations</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">nuclear matter aspects</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">quark deconfinement</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">quark-gluon plasma production</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">phase-transition</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">neutron star crust</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">meson interactions</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">quantum molecular dynamics</subfield></datafield><datafield tag="776" ind1=" " ind2=" "><subfield code="z">3-0365-5399-1</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Negreiros, Rodrigo</subfield><subfield code="4">edt</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Dexheimer, Veronica</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Negreiros, Rodrigo</subfield><subfield code="4">oth</subfield></datafield><datafield tag="906" ind1=" " ind2=" "><subfield code="a">BOOK</subfield></datafield><datafield tag="ADM" ind1=" " ind2=" "><subfield code="b">2023-12-15 05:40:00 Europe/Vienna</subfield><subfield code="f">system</subfield><subfield code="c">marc21</subfield><subfield code="a">2022-11-05 21:33:14 Europe/Vienna</subfield><subfield code="g">false</subfield></datafield><datafield tag="AVE" ind1=" " ind2=" "><subfield code="i">DOAB Directory of Open Access Books</subfield><subfield code="P">DOAB Directory of Open Access Books</subfield><subfield code="x">https://eu02.alma.exlibrisgroup.com/view/uresolver/43ACC_OEAW/openurl?u.ignore_date_coverage=true&portfolio_pid=5340568150004498&Force_direct=true</subfield><subfield code="Z">5340568150004498</subfield><subfield code="b">Available</subfield><subfield code="8">5340568150004498</subfield></datafield></record></collection> |