Hunting for Glitches Sarah Buchner. …are the leftover cores from supernova explosions. Almost...
-
Upload
eleanor-weaver -
Category
Documents
-
view
230 -
download
0
Transcript of Hunting for Glitches Sarah Buchner. …are the leftover cores from supernova explosions. Almost...
Hunting for Glitches
Sarah Buchner
• …are the leftover cores from supernova explosions. • Almost black holes• Neutron stars are very dense (1017 kg/m3 )
– 1.5 M with a diameter of 10 to 20 km
– Mass 1027 tons
• They rotate very rapidly: Period = 1.3 ms to 8 sec• magnetic fields are 1013 times stronger than Earth’s.
Neutron Stars
Chandra X-ray image of the neutron star left behind by a supernova observed in A.D. 386.The remnant is known as G11.20.3.
Pulsars and Neutron Stars
The Pulsar
Vela Pulsar
• PSR 0833-45• Vela supernova remnant• About 10 000 years old• P = 0.089 s = 11.2 Hz
• HartRAO observed • most days since 1984
Pulsars – stable clock• Massive stable flywheels superb cosmic clocks
e.g. Vela:
Unambiguously number each pulse
There were exactly 47 414 570 pulses between
11 Mar 2004 20:55:37and
29 Apr 2004 21:41:37
OH masers
Source below
horizon
VLBI
1s.Hz
-1310(6)-156.20475
Hz 00910.000000005181711.1910720
Phase residuals
Glitch Detection
• When phase offset > limit• Continual observing begins • Alarm at HartRAO• sms observers• Astronomical telegram / IAU circular
Spin-upnu
-5
0
5
10
15
20
25
30
35
0 10 20 30 40 50 60 70 80 90
MJD 48437
nu
x 1
E6
610715.2
Recovery
-25
-20
-15
-10
-5
0
5
0 10 20 30 40 50 60 70 80 90
MJD 48437
nu
do
t
Recovery time scales0.4 and 4.1 days
Cause of glitch - starquake
R
R2
I
I
//=10=10––66
ε = 10= 10-4
//=10=10––66
ε = 10= 10-4
Vortex pinning and unpinning
Vortex pinning
Vortex current depends on lag
Glitch
SSCC II
Spin-upnu
-5
0
5
10
15
20
25
30
35
0 10 20 30 40 50 60 70 80 90
MJD 48437
nu
x 1
E6
610715.2
Linear coupling “resistive”
Crust
Pinned superfluid
Next
Nint
Nint
coupleextcc NNI
)(I
N CSCcouple
)(I
NI CSCextCC
)(I
I CSCSS
Simple model
Spin-down
Non-linear coupling “capacitive”
Post-glitch recovery
n
t
n0)( ett pp
pd)( dtet
Recoveries have same form?
Predicting glitches
But …..
Do glitches occur randomly?
Size of angular momentumreservoir
Slope sets a lower limit to
IIres
Crab vs Vela
96 1010 910
How fast does the crust spin up?
Can we catch a glitch in the act?
XDMObservations
Timing Vela with XDM
Thanks
• HartRAO workshop staff and astronomers
• Adriaan Hough
• Richard Lord
• Simon Ratcliffe