The magnetar SGR 1935+2154 is reported to have an anti-glitch,accompanied by fast radio bursts,and transient pulsed radio emission.In the wind braking model,this triplet event tells people that(1) SGR 1935+2154 does n...The magnetar SGR 1935+2154 is reported to have an anti-glitch,accompanied by fast radio bursts,and transient pulsed radio emission.In the wind braking model,this triplet event tells people that(1) SGR 1935+2154 does not have a strong particle wind and can be approximated by magnetic dipole braking in the persistent state;(2) its antiglitch is due to an enhanced particle wind,similar to the first anti-glitch in magnetars;(3) its transient pulsed radio emission may be due to a decreasing emission beam during the outburst;(4) the enhanced particle acceleration potential and pulsar death line may not be the dominate factor.展开更多
Recently another long period radio pulsar GPM J1839-10 has been reported,similar to GLEAM-X J162759.5-523504.3.Previously,the energy budget and rotational evolution of long period radio pulsars had been considered.Thi...Recently another long period radio pulsar GPM J1839-10 has been reported,similar to GLEAM-X J162759.5-523504.3.Previously,the energy budget and rotational evolution of long period radio pulsars had been considered.This time,the death line and pulse width for neutron star and white dwarf pulsars are investigated.The pulse width is included as the second criterion for neutron star and white dwarf pulsars.It is found that:(1)PSR J0250+5854 and PSR J0901-4046 etc.should be normal radio pulsars.They have narrow pulse width and they lie near the radio emission death line.(2)The two long period radio pulsars GLEAM-X J162759.5-523504.3 and GPM J1839-10 are unlikely to be normal radio pulsars.Their possible pulse width is relatively large.They lie far below the fiducial death line on the P-P^(·)diagram.(3)GLEAM-X J162759.5-523504.3 and GPM J1839-10 may be magnetars or white dwarf radio pulsars.At present,there are many parameters and uncertainties in both of these possibilities.展开更多
基金supported by the National SKA Program of China(No.2020SKA0120300)NSFC(12133004)。
文摘The magnetar SGR 1935+2154 is reported to have an anti-glitch,accompanied by fast radio bursts,and transient pulsed radio emission.In the wind braking model,this triplet event tells people that(1) SGR 1935+2154 does not have a strong particle wind and can be approximated by magnetic dipole braking in the persistent state;(2) its antiglitch is due to an enhanced particle wind,similar to the first anti-glitch in magnetars;(3) its transient pulsed radio emission may be due to a decreasing emission beam during the outburst;(4) the enhanced particle acceleration potential and pulsar death line may not be the dominate factor.
基金supported by National SKA Program of China(No.2020SKA0120300)the National Natural Science Foundation of China(NSFC,12133004)。
文摘Recently another long period radio pulsar GPM J1839-10 has been reported,similar to GLEAM-X J162759.5-523504.3.Previously,the energy budget and rotational evolution of long period radio pulsars had been considered.This time,the death line and pulse width for neutron star and white dwarf pulsars are investigated.The pulse width is included as the second criterion for neutron star and white dwarf pulsars.It is found that:(1)PSR J0250+5854 and PSR J0901-4046 etc.should be normal radio pulsars.They have narrow pulse width and they lie near the radio emission death line.(2)The two long period radio pulsars GLEAM-X J162759.5-523504.3 and GPM J1839-10 are unlikely to be normal radio pulsars.Their possible pulse width is relatively large.They lie far below the fiducial death line on the P-P^(·)diagram.(3)GLEAM-X J162759.5-523504.3 and GPM J1839-10 may be magnetars or white dwarf radio pulsars.At present,there are many parameters and uncertainties in both of these possibilities.
