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Pulsars

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You are listening to a radio recording of a pulsar (the Vela pulsar) of mass ... parameters have been obtained; precession due to relativistic spin-orbit ... – PowerPoint PPT presentation

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Title: Pulsars


1
Pulsars progress and puzzles
  • Jocelyn Bell Burnell
  • University of Oxford Astrophysics
  • Mansfield College

2
Audio recording of a pulsar
  • You are listening to a radio recording of a
    pulsar (the Vela pulsar) of mass 1027 tonnes
    spinning on its axis 11 times a second.

Vela SN remnant
3
Pulsars - a fast pulsar
  • The fastest known pulsar used to be
  • PSR193721, with a period of
  • P 1.5578064688197945/-
    0.0000000000000004 ms
  • The current fastest has a period 1.396 ms
  • Question how fast can a pulsar spin?

4
Pulsar model
  • Star spins like a lighthouse, sweeping radio beam
    around the sky.
  • We see a pulse each time beam sweeps across us.

5
Pulsar timing
  • Their accurate timekeeping means
  • Pulsars can be used as clocks to test Einsteins
    Theory of Relativity.
  • Binary orbits can be studied precisely
  • Progress the 5 post-Keplerian parameters have
    been obtained precession due to relativistic
    spin-orbit coupling has been reported.
  • Doppler shifts can reveal presence of planets
  • Puzzle why one and only one system with
    planets?

6
Pulsar test of GR
  • The orbit of the Binary Pulsar shrinks exactly as
    predicted by Einstein.
  • It implies that gravitational radiation exists as
    predicted by Einstein.

7
Pulsars an amazing fact
  • The roundest known thing in the universe is the
    orbit of a pulsar around its companion star. It
    is round to 1 micron in 100000km.
  • Information obtained from Doppler shifts as
    pulsar orbits.

8
Magnetic field
  • Assuming magnetic dipole radiation
  • Magnetic field is 108 Tesla (1010 - 10 11Tesla in
    magnetars)
  • Questions
  • How is magnetic field created?
  • How is it sustained?
  • What shape is it?

9
Pulsars radio emission
  • They are weak emitters of radio waves
  • Question how and where is the radio emission
    produced? (Magnetic pole)
  • Intermittent pulsars have recently been
    discovered.
  • How do you make an intermittent pulsar?

10
Mass and density of pulsars
  • Mass 1027 tonnes
  • Radius 10 km
  • Average density density of nucleus
  • Squeeze the 6 billion people
  • that inhabit Earth into a thimble
  • and it has the same mass as a
  • thimble full of neutron star material

11
Mass and density contd
  • Question what is range of allowable masses?
  • Not known, but hints of masses as large as
    1.8MSun - this could require different
    structure.
  • Progress physics of very condensed matter now
    better understood. Structure of neutron star
    being studied.

12
Rigid crust of
Fe56 atoms
Neutron- rich
nuclei
Neutron
superfluid Core solid? liquid? Hyperons? Quarks?
Possible structure of a neutron star
of a neutron starStructure
13
Pulsars an amazing fact
  • If you drop a coin on to the surface of a neutron
    star, it will hit the surface with a speed of
    0.6c

14
Pulsar H-R diagram
  • Pulsar P dP/dt plot
  • TG TeraGauss field derived assuming magnetic
    dipole radiation.
  • Age estimated from current rate of evolution

dP/dt
Period (s)
15
Pulsar H-R diagram
  • Pulsar formed in SN explosion (core collapse or
    electron capture).
  • Appears upper-centre of this diagram.
  • Evolves down and to right, and becomes
  • radio quiet.
  • Pulsar in binary spun-up again and
  • reappears as ms pulsar.
  • Puzzle
  • Magnetars - top right B 1014 G
  • Progress

dP/dt
Period (s)
16
Conclusions
  • Field keeps re-inventing itself still full of
    drama!
  • Current issues
  • Magnetars
  • Intermittent pulsars
  • Testing GR and alternatives
  • Pulsar timing array to detect Grav Radiation
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