Title: Review: How does a star
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2Supernovae and nucleosynthesis of elements gt Fe
3Death of low-mass star White Dwarf
- White dwarfs are the remaining cores once fusion
stops - Electron degeneracy pressure supports them
against gravity - Cool and grow dimmer over time
4A white dwarf can accrete mass from its companion
5Tychos supernova of 1572
6Expanding at 6 million mph
7Keplers supernova of 1609
8Supernovae outshine the whole galaxy!
9Two kinds of supernovae
Type I White dwarf supernova White dwarf near
1.4 Msun accretes matter from red giant
companion, causing supernova explosion Type II
Massive star supernova Massive star builds up
1.4 Msun core and collapses into a neutron star,
gravitational PE released in explosion
10light curve shows how luminosity changes with
time
11r process and s process elements
- Nuclear fusion in all stars only produces up to
Fe-56 - Slow neutron capture (s process) forms up to
Bi-209 in low-mass stars - High temps in SN creates elements up to Ca-254
- Rapid neutron capture (r process) create
neutron-rich isotopes which decay into more
stable neutron-rich elements - Neutron flux during SN is 1022 neutrons per
square centimeter per second - neutron captures occur much faster than decays
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13A neutron star A few km in diameter, supported
against gravity by degeneracy pressure of neutrons
14Discovery of Neutron Stars
- Using a radio telescope in 1967, Jocelyn Bell
discovered very rapid pulses of radio emission
coming from a single point on the sky - The pulses were coming from a spinning neutron
stara pulsar
15Pulsar at center of Crab Nebula pulses 30 times
per second
16Pulsars
17Thought Question
- Could there be neutron stars that appear as
pulsars to other civilizations but not to us? - A. Yes
- B. No
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18Thought Question
- Could there be neutron stars that appear as
pulsars to other civilizations but not to us? - A. Yes
- B. No
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19What happens if the neutron star has more mass
than can be supported by neutron degeneracy
pressure?
- It will collapse further and become a black hole
- It will spin even faster, and fling material out
into space - Neutron degeneracy pressure can never be overcome
by gravity
20- Neutron degeneracy pressure can no longer support
a neutron star against gravity if its mass is gt
about 3 Msun
2118.3 Black Holes Gravitys Ultimate Victory
A black hole is an object whose gravity is so
powerful that not even light can escape it.
22Escape Velocity
Final Gravitational Potential Energy
Initial Kinetic Energy
Where m is your mass, M is the mass of the
object that you are trying to escape from, and r
is your distance from that object
23Light would not be able to escape Earths surface
if you could shrink it to lt 1 cm
24Surface of a Black Hole
- The surface of a black hole is the distance at
which the escape velocity equals the speed of
light. - This spherical surface event horizon.
- The radius of the event horizon is known as the
Schwarzschild radius.
25Neutron star
The event horizon of a 3 MSun black hole is a
few km
26A black holes mass strongly warps space and time
in vicinity of event horizon
27What would it be like to visit a black hole?
28Light waves take extra time to climb out of a
deep hole in spacetime, leading to a
gravitational redshift
29Time passes more slowly near the event horizon
30Thought Question
- Is it easy or hard to fall into a black hole?
- A. Easy
- B. Hard
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31Tidal forces near the event horizon of a 3 MSun
black hole would be lethal to humans Tidal
forces would be gentler near a supermassive black
hole because its radius is much bigger
32Do black holes really exist?
33Black Hole Verification
- Need to measure mass
- Use orbital properties of companion
- Measure velocity and distance of orbiting gas
- Its a black hole if its not a star and its mass
exceeds the neutron star limit (3 MSun)
34Some X-ray binaries contain compact objects of
mass exceeding 3 MSun which are likely to be
black holes
35One famous X-ray binary with a likely black hole
is in the constellation Cygnus
36Thought Question
- How does the radius of the event horizon change
when you add mass to a black hole? - A. Increases
- B. Decreases
- C. Stays the same
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37Thought Question
- How does the radius of the event horizon change
when you add mass to a black hole? - A. Increases
- B. Decreases
- C. Stays the same
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38Thought Question
- Is it easy or hard to fall into a black hole?
- A. Easy
- B. Hard
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Hint A black hole with the same mass as the Sun
wouldnt be much bigger than a college campus
39Thought Question
- Is it easy or hard to fall into a black hole?
- A. Easy
- B. Hard
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Hint A black hole with the same mass as the Sun
wouldnt be much bigger than a college campus
40If the Sun shrank into a black hole, its gravity
would be different only near the event horizon
Black holes dont suck!
41Event horizon is larger for black holes of larger
mass Black holes have only mass, spin and charge