Počet záznamov: 1
On cooling of neutron stars with a stiff equation of state including hyperons
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$a 10.1016/j.nuclphysa.2018.10.014 $2 DOI 035 $a biblio/93811 $2 CREPC2 100 $a 20181212d2018 m y slo 03 ba 101 0-
$a eng 102 $a CH 200 1-
$a On cooling of neutron stars with a stiff equation of state including hyperons $f Hovik Grigorian, Evgeni E. Kolomeitsev ... [et al.] 330 0-
$a Exploiting a stiff equation of state of the relativistic mean-field model MKVORHf with sigma-scaled hadron effective masses and couplings, including hyperons, we demonstrate that the existing neutron-star cooling data can be appropriately described within “the nuclear medium cooling scenario” under the assumption that different sources have different masses 463 -1
$1 001 umb_un_cat*0289894 $1 011 $a 2218-1997 $1 200 1 $a Universe $v Vol. 4, no. 2 (2018), pp. 1-6 $1 210 $a Basel $c Multidisciplinary Digital Publishing Institute $d 2018 606 0-
$3 umb_un_auth*0247154 $a equation of state 606 0-
$3 umb_un_auth*0221939 $a neutron stars 606 0-
$3 umb_un_auth*0298406 $a neutrína $X neutrinos 615 $n 53 $a Fyzika 675 $a 53 700 -1
$3 umb_un_auth*0272897 $a Grigorian $b Hovik $4 070 $9 25 701 -1
$3 umb_un_auth*0131258 $a Kolomeitsev $b Evgeni E. $p UMBFP06 $4 070 $9 25 $f 1970- $T Katedra fyziky 701 -1
$3 umb_un_auth*0258764 $a Maslov $b Konstantin A. $9 25 $4 070 701 -1
$3 umb_un_auth*0160605 $a Voskresensky $b Dmitri $4 070 $9 25 801 $a SK $b BB301 $g AACR2 $9 unimarc sk 856 $u https://www.mdpi.com/2218-1997/4/2/29 $a Link na zdrojový dokument T85 $x existuji fulltexy
Počet záznamov: 1