Overview of Stellar Evolution
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1 Overview of Stellar Evolution
2 Walter Baade With Fritz Zwicky first proposed that neutron stars could be formed by supernovae in 1934 Iron core collapse E+p->n+ Degenerate neutrons limit size to 3 solar masses
3 A One Solar Mass Neutron Star is the size of Victoria Neutron star ~10km diameter Distance from downtown to Mt Doug Black Hole 3km UVic- Mt. Tolmie
4 Model of Neutron Star Over Chandrasekhar limit of 1.4 M sun Radius decreases 10 5 X to 10km so density increases X Spin increases times so rotation from 25d to millisec
5 Model of Neutron Star Temperature of Millions K Magnetic field increases to gauss (Fridge magnet ~100 g) Convection currents in millisecs
6 Hard to Detect Nearest Neutron Star 180 light years 700,000K 20km diameter Small luminosity Plowing through ISM At 200km/sec forming A bow shock of recombining hydrogen
7 Jocelyn Bell Discovered pulsars in 1967 While using new radio telescope in Cambridge UK Discovered Crab pulsar in 1968
8 Pulsar Model Rapidly rotating neutron star Magnetic field inclined to rotation axis Relativistic charged particles trapped by magnetic field beam light along field lines
9 Parks Movie of Lighthouse Model Neutron star rotates and beams come from magnetic axis Spinning magnetic field generates electric field accelerating charged particles
10 Pulsar Pulses Spin rate = pulse periods range from to 3.75 seconds White Dwarf would fly apart if spun this fast Precision equal to atomic clock implies massive object Vela pulsar exploded ~11,000 years ago
11 Pulsar Profiles Pulse duration of about a millisec Emitter must be less than 300km in size Pulses seen at all wavelengths but most easily at radio Sometimes strong and weak pulses Crab pulsar on/off
12 Crab Movie: X-Ray &Visible Pulsar wind (like solar wind) energizes the nebula by carrying away the rotational energy of the pulsar
13 Pulsar Glitches Lost rotational energy observed as periods increasing Glitch is abrupt period decrease (Vela shown in graph) Caused by starquakes (1 cm) or fluid interior loosely coupled to crust? Pulsars spin down in millions of years
14 Pulsar Distribution Thousand discovered Millions in galaxy Mostly in galactic plane =Milky Way Most neutron stars not pulsars : spun down or wrong tilt
15 Personal point of view Observer point of view
16 Neutron Star in IC443 Summer High School students Using Chandra X-ray data Found neutron star offset from center of SNR Most pulsars not in remnants and lots of SN remnants have no pulsar. Why????
17 Why are Pulsars NOT Found in SNR? Large proper motions Asymmetric explosions? Not in SNR which last ~ 50,000 years Pulsars slow down in 10 Million years Binary star???
18 Fastest Millisecond Pulsar Spun up by mass from companion Discovered by J. Hessels McGill Rotates at 716 Hz = a blender It is less than 16 km radius. Found in Globular Cluster; old star Figure shows pulsar ablating companion which eclipses pulsar
19 Pulsar PSR s Planets Planet masses from mutual interactions: 2 ~Earths, 1 ~moon mass Orbit so close to pulsar they should have been destroyed in explosion
20 Binary Pulsar PSR Discovered 1974; Nobel prize for Taylor&Hulse in 1993 Orbital Period ~8 hours One pulsar & the other a neutron star= 1.35 solar mass Slows due to Gravitational Radiation predicted by General Relativity Orbit shrinks 3mm/year so they will merge in 300 million years
21 Maybe Merging Neutron Stars ~30,000 binary neutron stars and 300 black hole binaries 2 stars 1.4 solar masses are 30km diameter and 10km apart This is a cut-away showing the insides
22
23 Special Relativity st Postulate Observers can never detect their uniform motion except relative to other objects 1 st Postulate Physical laws are the same for all observers 2 nd Postulate The velocity of light is a constant and will be the same for all observers independent of their motion relative to the light source E=Mc 2
24 Special Relativity Time Dilation Red & Blue make identical clocks from light pulses & mirrors If Blue moves near the speed of light his clock runs slower relative to Red s because his light pulses need to travel farther Make a time machine to slow time and travel to the future
25 Twin Paradox
26 General Relativity 1916 Equivalence principle: Observers cannot distinguish locally between inertial forces due to acceleration and uniform gravitational forces due to the presence of a massive body. (Light Too)
27 Precession of Mercury s Orbit General Relativity theory correctly predicts the observation of the precession of Mercury s orbit Newtonian gravity in red is incorrect and Einstein s in blue A theory can not be proven correct only shown to be incorrect
28 Gravitational Bending of Light Positions of stars seen during a solar eclipse are displaced as predicted by General Relativity; 1919
29 General Relativity Time Dilation General Relativity predicts that Acceleration/gravity makes clock run more slowly Seen in GPS s Again you can make a time machine to travel to the future
30 Gravitational Redshift As light climbs out of gravitational potential well it loses energy It can not slow down so it must redshift Has been seen for Sun, White Dwarfs and on Earth
31 Black Hole Formation
32 Karl Schwarzschild First solution to General Relativity equations for Black Hole Escape velocity of : Earth=11km/sec, Sun=600km/sec, white dwarf= 10,000km/sec, neutron star= 100,000km/sec At event horizon escape velocity =c Schwarzschild radius R s =2GM/c 2 1 Earth Mass -> 1cm 1 Solar Mass -> 3km Radius in km R s =3 M in solar masses 10 Solar Masses -> 30km
33 Schwarzschild Radius=Event Horizon Singularity is where R=0 F=GMm/R 2 becomes infinite Only observable properties are Mass, Charge, Rotation If sun replaced by BH- no change in orbits
34 Kerr Black Hole When stars collapse they are rotating so the remnant black hole should rotate fast Event horizon becomes oblate spheroid Ergosphere- area where space-time rotates with black hole
35 Gravitational Redshift BH As light comes out of a Black Hole it looses energy and thus redshifted At Event Horizon light infinitely redshifted
36 Black Hole Lens in Orion Black hole bends light Two images appear, one on either side
37 Black Hole Evaporation Black Holes do seem to radiate energy The smaller the hole the hotter it seems primordial? A 1 Solar mass black hole will last ~10 70 years
38 Falling into a Black Hole 4. Tides heat him to millions K 5. Clock A would stop as he reached event horizon 6. Person A would notice nothing unusual at event horizon
39 Evidence for Black Holes: Cygnus X-1 O-type Supergiant >3.8M sun Black Hole 5.6d orbital period X-rays flicker in 0.01sec 10 systems known
40 SS433 s Jets; Black Holes are Messy Eaters 16,000ly distant Eclipses every 13 days Star is 13 M sun Interaction of magnetic fields of accretion disk and compact object ejects jets at 0.25 c Precesses in 164 days Seen in X-rays and radio Black hole is 3-8 M sun
41 Quasi-Periodic Oscillations A mass falling into a black hole will release 100 times as much energy as could be obtained from fusion
42 X-Ray Binary X-ray binary containing a Black Hole will be fainter than one containing a neutron star No terminal burst
43 Painting of Black Hole
44
45 Compton Observatory Vela 1968 designed to detect nuclear bomb tests Beppo-Sax 1997 could pinpoint burst SWIFT detects about 1 a day
46 Gamma Ray Burst Animation
47 Gamma Ray Burst Light Curves Duration of seconds sets upper limit to size of hundreds of thousands of kilometers Like a pulsar pulse
48 Gamma Ray Burst Distribution No concentration to: Sun, Sirius, Crab, galactic plane, galactic center, Andromeda galaxy, Virgo Cluster
49 Power of Gamma Ray Bursts Brighter than all the stars in universe for a second ergs is mass of sun totally converted to energy Beaming reduces energy but increases frequency
50 Maybe Beamed - Hypernova Similar to core collapse supernovae but ~30 solar mass WR star Core collapses to form Black Hole, accretion disc forms, jets form, eventually blast through surface of star, hit surrounding material, creates gamma rays
51 GRB Effects on Earth Nearest binary pulsar ~1600ly=10 4 megatn Occur every few hundred(?) million years
52
53 Review of Black Holes & Pulsars What happens when a star contracts? S m t What are pulsars? How do we know they are small? What is a Black Hole? E 3/1 What happens if you fall into one? R t t Why do we think they exist? 2 & X
54 Millisecond Pulsar Top View At the distance of the moon from the Earth the magnetic field rotates at speed of light
55 Millisecond Pulsar Surface Rotates at the speed of a blender
56 Falling into BH Movie 30 Solar Mass BH Done by Andrew Hamilton From 1 AU takes 65 days No redshift
57 X-ray Burster Carbon (or helium) builds up on surface of neutron star Which eventually explodes like a nova Illuminating disk Observed by Dave Ballantyne with ROSSI Explorer
58 GRB Light Echo in X-Rays X-Rays emitted during a GRB reflect off a dust cloud 3500ly from Earth in our Galaxy So it is beyond the dust cloud
59 Planet and White Dwarf Orbit Millisecond Pulsar
60 XTE Black Hole & Solar Mass Star
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