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Transcript
Extracting Energy from a BH
•  Rotational energy stored in ergosphere
–  Can be extracted
•  Penrose process:
–  mass falls in, splits in two
–  Half falls in, half falls out
with more energy
Extracting Energy from a BH
•  Blandford-Znajek process:
–  Magnetic field threads ergosphere
–  Plasma travels along field lines, is accelerated
in ergosphere
Gravitational Waves
• 
• 
• 
• 
Gravitational radiation
Binary inspiral
Evidence for gravity waves
Methods for direct detection
Gravitational Radiation
•  Gravity moves at the speed of light
•  Change is how mass is arranged
communicated out at speed of light
Electromagnetic Radiation
•  When charge is accelerated, it produces
light
Gravitational Radiation
•  Only one charge in gravity, so no dipole
radiation
•  But, quadrupole moment can change and
produce gravitational radiation
Gravitational Radiation
•  Only one charge in gravity, so no dipole
radiation
•  But, quadrupole moment can change and
produce gravitational radiation
•  Mass distribution must be asymetric
Sources of gravitational waves
•  Supernovae – asymmetric explosion
Sources of gravitational waves
•  Supernovae – asymmetric explosion
•  Binary stars, neutron stars, black holes
Sources of gravitational waves
•  Supernovae – asymmetric explosion
•  Binary stars, neutron stars, black holes
•  Merging neutron stars, black holes
Sources of gravitational waves
•  Merging neutron stars
Sources of gravitational waves
•  Merging neutron stars
Sources of gravitational waves
•  Merging
black holes
Sources of gravitational waves
•  Merging
black holes
Gravitational Waves
•  Gravitational waves carry away energy and
angular momentum
•  Eventually gravitational radiation will cause
a binary to merge
Evidence for gravitational waves
•  Pulsar binaries
•  Pulsar in orbit with a neutron star of white
dwarf
•  Pulse period changes due to doppler shift as
it orbits
Evidence for gravitational waves
•  Pulsar binaries
•  Pulsar in orbit with a neutron star of white
dwarf
•  Pulse period changes due to doppler shift as
it orbits
•  Over time, orbit gets closer, orbital period
decreases
Evidence for gravitational waves
•  PSR B1913+16
•  Discovered by
Russell Hulse and
Joseph Taylor in
1974
•  Won Nobel Prize in
1993
Direct detection
•  As gravitational waves goes by, is stretches
space
•  Distance between points changes
Methods for direct detection
•  Need something of fixed size you can
measure changes in
Methods for direct detection
•  Need something of fixed size you can
measure changes in
•  Gravitational waves will set off vibrations
in a solid mass
Methods for direct detection
•  Need something of fixed size you can
measure changes in
•  Laser interferometer:
–  2 beams of fixed length, at 90 degrees to each
other
–  Interference pattern will change if length of
arms changes
LIGO
LIGO
•  2 detector – Louisiana and Washington
–  3000 km apart
•  4 km arms
LISA
•  Space interferometer
LISA
LISA