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Black Holes
Underlying principles of General Underlying principles of General RelativityRelativity
The Equivalence Principle
No difference between a steady acceleration and a gravitational field
Gravity and Acceleration cannot be distinguished
h
V = a h/c
h Gravitational field
Equivalence principle – this situation should be the same
Principe May 1919
Eddington tests General Relativity and spacetime curvature
GR predicts light-bending of order 1 arcsecond near the limb of the Sun
Lensing of distant galaxies by a foreground cluster
QSO 2237+0305
The Einstein cross
Curved Space: A 2-dimensional analogy
Flat space
Angles of a triangle add up to 180 degrees
Radius r
Circumference of a circle is 2πr
Positive and Negative Curvature
Triangle angles >180 degrees
Circle circumference < 2πr
Triangle angles <180 degrees
Circle circumference > 2πr
The effects of curvature only become noticeable on scales comparable to the radius of curvature. Locally, space is flat.
A geodesic – the “shortest possible path”** a body can take between two points in spacetime (with no external forces). Particles with mass follow timelike geodesics. Light follows “null” geodesics.
** This is actually the path that takes the maximum “proper” time.
Space
Time
Spacelike
Timelike
Curved geodesic caused by acceleration OR gravity
Matter tells space(time) how to curve
Spacetime curvature tells matter how to move
Mass (and energy, pressure, momentum) tell spacetime how to curve;
Curved spacetime tells matter how to move
A formidable problem to solve, except in symmetric cases – “chicken and egg”
Curvature of space in spherical symmetry – e.g. around the Sun
h
V = (2ah)1/2
Special Relativity
A moving clock runs slow
Observer ON TRAIN Observer BY TRACKSIDE
Speed of light is c=300,000 km/s
t’ = 2d / c
Width of carriage
Is d meters
Train speed v
d
vt/2
s
t = 2s / cSo t’ is smaller than t
Observers don’t agree! Smaller by a factor
Where v2/c2)
h
V = (2ah)1/2
Special Relativity
A moving ruler is shorter
h
Gravitational field
According to the equivalence principle, this is the same as
Curvature of space in spherical symmetry – e.g. around the Sun
Spacetime curvature near a black hole
A black hole forms when a mass is squashed inside it’s Schwarzschild Radius RS = 3 (M/Msun) km
Time dilation factor
1/(1 – RS/r)1/2
Becomes infinite when r=RS
Remnant < 1.4 M
Progenitor < 8 M
White Dwarf
Planetary Nebula
A cooling C/O core, supported by quantum mechanics! Electron degeneracy pressure.
The Chandrasekhar limit
Cools forever – gravity loses!
Progenitor > 8 M
Black Hole – gravity wins!
Supernova
Neutron star, supported by quantum mechanics! Neutron degeneracy pressure.
Cools forever – gravity loses!
Remnant < 2.5 M Remnant > 2.5 M
20 km
Black Holes in binary systems
M3 sin3i = 0.25 (M + m)2 Period = 6 days
Cygnus X-1
M > 5 Msun
Ellipsoidal light curve variations
Depend on mass ratio and orbit inclination
BH mass
Black hole mass 10 –15 x Msun
Combine ellipsoidal model with radial velocity curve
Spinning black holes – the Kerr metric
Spaghettification
A 10g stretching force felt at 3700 km (>RS) from a 10 Msun black hole
Force increases as 1/r3
Supermassive Black Holes
Jets propelled by twisted magnetic field lines attached to gas spiralling around a central black hole
Supermassive Black Hole in the Galactic Centre
Mass is 4 millions times that of the Sun
Schwarzschild radius 12 million km = 0.08 au
Falling into a black hole