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Mechanism of r-mode stability in young rapidly rotating pulsars
Title Mechanism of r-mode stability in young rapidly rotating pulsars Author info E. E. Kolomeitsev, D. N. Voskresensky Author Kolomeitsev Evgeni E. 1970- (50%) UMBFP06 - Katedra fyziky
Co-authors Voskresensky Dmitri (50%)
Source document The European Physical Journal A : Hadrons and Nuclei. Vol. 50, no. 12 (2014), pp. [1-5]. - Berlin : Springer, 2014 Keywords r-modes viscosity neutron stars young pulsars Language English Country Germany systematics 53 Annotation We demonstrate that stability of r-modes in young rapidly rotating pulsars might be explained if one takes into account strong medium modifications of the nucleon-nucleon interaction because of the softening of pionic degrees of freedom in dense nucleon matter. Presence of the efficient direct Urca processes is not required. Within our model the most rapidly rotating observed young pulsar PSR J0537-6910 should have the mass > 1.8M_sol Public work category ADC No. of Archival Copy 31379 Catal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Database xpca - PUBLIKAČNÁ ČINNOSŤ References PERIODIKÁ-Súborný záznam periodika 
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Number of the records: 1