MATHEMATICAL MODEL FOR GLITCHES IN PULSARS

被引：1
|
作者：
Mongiovi, M. S. [1 ]
Sciacca, M. [1 ]
机构：
[1] Univ Palermo, Dipartimento Metodi & Modelli Matemat, I-90128 Palermo, Italy
来源：
WASCOM 2009: 15TH CONFERENCE ON WAVES AND STABILITY IN CONTINUOUS MEDIA | 2010年
关键词：
Neutron star; superfluidity; NEUTRON-STAR; CORE;
D O I：
10.1142/9789814317429_0040
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The aim of this work is to propose a simple mathematical model which is able to capture the peculiar behaviour of the rotating neutron star: glitches. This is made by using the knowledge on helium superfluid and particularly on rotating superfluid helium, which has interested many researchers over the years.
引用
收藏
页码：297 / 302
页数：6
相关论文
共 50 条
  • [1] Pulsars, glitches and superfluids
    Alpar, MA
    PHYSICS WORLD, 1998, 11 (01) : 25 - 26
  • [2] Glitches in the rotation of pulsars
    Espinoza, Cristobal
    Lyne, Andrew
    Stappers, Ben
    Kramer, Michael
    RADIO PULSARS: AN ASTROPHYSICAL KEY TO UNLOCK THE SECRETS OF THE UNIVERSE, 2011, 1357 : 117 - 120
  • [3] Simulations of glitches in pulsars
    Larson, MB
    Link, B
    RELATIVISTIC ASTROPHYSICS, 2001, 586 : 553 - 555
  • [4] Glitches in southern pulsars
    Wang, N
    Manchester, RN
    Pace, R
    Bailes, M
    Kaspi, VM
    Stappers, BW
    Lyne, AG
    PULSAR ASTRONOMY - 2000 AND BEYOND: IAU COLLOQUIUM 177, 2000, 202 : 109 - 110
  • [5] Glitches in southern pulsars
    Wang, N
    Manchester, RN
    Pace, RT
    Bailes, M
    Kaspi, VM
    Stappers, BW
    Lyne, AG
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2000, 317 (04) : 843 - 860
  • [6] Simulations of glitches in isolated pulsars
    Larson, MB
    Link, B
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2002, 333 (03) : 613 - 622
  • [7] 30 glitches in slow pulsars
    Janssen, G. H.
    Stappers, B. W.
    ASTRONOMY & ASTROPHYSICS, 2006, 457 (02): : 611 - 618
  • [8] 30 glitches in slow pulsars
    Janssen, G.H.
    Stappers, B.W.
    Astronomy and Astrophysics, 1600, 457 (02): : 611 - 618
  • [9] Properties and observability of glitches and anti-glitches in accreting pulsars
    Ducci, L.
    Pizzochero, P. M.
    Doroshenko, V.
    Santangelo, A.
    Mereghetti, S.
    Ferrigno, C.
    ASTRONOMY & ASTROPHYSICS, 2015, 578
  • [10] Mathematical model of glitches in DAC with weight redundancy
    Azarov, Olexiy D.
    Murashenko, Oleksandr G.
    Katsiv, Semen S.
    Gromaszek, Konrad
    Duskazaev, Gali
    Ussatova, Olga
    OPTICAL FIBERS AND THEIR APPLICATIONS 2018, 2019, 11045
12345