Lectures | Lecture page | Astro103 page |
What's standard?
mass for core-collapse (type II)
We are all made of star matter
- densities as high as atomic nuclei themselves
- one giant 'nuclei' -- bound by gravity
- high rotation speed
- spin rates as fast as 1000 times per second!
(surface spinning at 20% of speed of light)
------------------------- 1.4 M limit
neutron stars
------------------------- 3 M limit ???
black holes
Other possibilities before the inevitable limit: (remember the zoo!)
with ever-increasingly massive quarks:
'charm' matter
'bottom' matter
'top' matter
Introduce a new particle whenever the Fermi Seas get high enough to reach that particle's mass
Special Relativity:
(Recall, the speed of light is finite)
- Becomes Newton's ``Laws of Motion'' when speeds are much less than light speed
- Reformulates gravity as ``curvature'' in space and time
- Acceleration is when an object resists curvature
- ``Free-fall'' is an inertial frame
Special Relativity has been incorporated into Quantum Mechanics, but there is currently no theory of Quantum Gravity! (yet)
Where escape velocity = speed of light
Time dilation
Define:
increases (redder) gravitational redshift
= 1 / decreases time dilation
- So too is gravitational redshift and time dilation.
Before the Event Horizon, such material radiates enormous amounts of energy.
gamma-ray bursters ???
active galactic nuclei
(b) The most important stars are low-mass stars.
(c) There must have been at least one generation of stars before the Sun and Solar System were formed.
(d) Massive stars could not have produced this material since they would have destroyed the Sun.
(e) Super-novae today are constantly supplying the Solar System with new heavy elements.
(b) The limiting mass for a black hole would go down.
(c) The limiting mass for a black hole would stay the same.
(d) There would not be a black hole event horizon.
(e) Time dilation at the event horizon would change.
Lectures | Lecture page | Astro103 page |