BANG! Structure of a White Dwarf NO energy production gravity = degenerate gas pressure as it cools, becomes Black Dwarf. Lives of High Mass Stars

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Structure of a White Dwarf NO energy production gravity = degenerate gas pressure as it cools, becomes Black Dwarf Mass Limit for White Dwarfs S. Chandrasekhar (1983 Nobel Prize) -calculated max. mass (White Dwarf) M wd 1.4 M Chandrasekhar limit If total mass of star < 6 to 8 M (core < 1.4 M ) - star ends as a White Dwarf Low Mass star If total mass of star > 6 to 8 M (core < 1.4 M!!) - cannot form White Dwarf!! High Mass stars Lives of High Mass Stars (M star > 6-8 M ) star Early life is same as a Low Mass Star: - Formation Process / Protostar - Main Sequence Phase Key Differences from a Low Mass Star: more mass = more gravity = higher temps Each stage is much quicker Supergiant (High Mass) Core fusion stops - Core collapses and heats up! Fusion shell begins around core - Next fusion starts in core Outer layers expand and cool Hydrogen Fusion (Main Seq.) Helium Fusion Carbon Fusion Neon Fusion Oxygen Fusion Silicon Fusion Production of Iron High Mass Supergiant: Onion Ring Structure Core becomes 100% iron, fusion STOPS Iron is most stable element Cannot create energy from Iron - Iron must absorb energy to fuse - Iron must absorb energy to fission Then BANG!

Death of High Mass Supergiant - Iron core collapses - cannot form White Dwarf Sudden Collapse of Core - Core Collapses in 1/4 second! 10,000 km. less than 30 km - infalling material - moving 15% speed of light! - flood of neutrinos released Collapse stops suddenly - when neutrons crowded together - enormous shock wave rips through star => SUPERNOVA EXPLOSION!!! Entire envelope blasted into space Contains lots of heavy elements Excess energy from explosion allows fusion heavier than iron Supernova seen July 4, 1054 AD Today oday,, seen as "Crab Nebula" X-ray Image

25 Solar Mass Star: (core mass > 1.4 M ) Core becomes Neutron Star giant ball of neutrons ~20 miles across contains between 1.4 to ~3 M rotates very fast Neutron degeneracy stops collapse Conserves angular (rotational) momentum Can be observed as: Pulsar - first detected in 1967 - http://www.jb.man.ac.uk/~pulsar/education/sounds/sounds.html 35 Solar Mass Star: (core mass > 3 M ) Core collapses when fusion stops - NOTHING can stop collapse!! All matter crushed out of existence Becomes a Black Hole Gravity too strong for anything (even light) to escape Space and Time no longer exist - explained by Einstein's General Relativity Einstein: General Theory of Relativity - Gravity is a "curvature" or distortion of Spacetime Mass creates a "distortion" in space & time - "distortion" will affect anything moving through space - even LIGHT will be affected!! Black Holes A place where gravity is so strong: - NOTHING, not even light, can escape "BLACK" - escape velocity > the speed of light! A place spacetime is so distorted: there is a HOLE in space & time! Black Holes: - made up of NOTHING! - region of highly warped space & time Only measurable properties of Black Hole Mass, Electric Charge, Rotation

Structure of a black hole: Singularity: - the point where all the matter is compressed into - place of infinite spacetime curvature Event Horizon: - location where V escape = c Search for Black Holes - can look for material that is falling in - forms accretion disk, emits X-rays - X-ray binary system Event Horizon Singularity - inside "disconnected" from the rest of the universe - no information can ever get out Schwarzschild Radius: - the radius of the event horizon Black Hole Candidates (1996) Object Companion Star Orbital Period (days) Mass of Compact Object (M o) Cyg X-1 X O9.7 I 5.6 11 LMC X-3 X B3 V 1.7 7.6 LMC X-1 X O7 V 4.2 7 A 0620-00 00 K5 V 0.32 2.9 GS 2023+338 G9 V-K0 III 6.47 6.1 GS 1124-68 K0 V-K4 V 0.43 2.9 GRO J0422+32 M2 0.21 4.8 GRO J1655-40 F3-F6 2.60 3.2 GS 2000+25 K5 V 0.35 6.4 H1705-25 K3 0.52 (0.70) 3.4 Astrophysical Journal Letters, 1996 2004, Black Hole Candidates: - 54 in binary systems - 4 by gravitational microlensing 2013, Chandra X-ray Observatory - 26 new candidates in Andromeda Galaxy Supermassive Black Holes At the center of galaxies, - large rotating disks of stars and gas - can calculate gravity needed to keep disk together 10 6 M o to 10 9 M o!! - size of region that provides gravity - much less than 1 pc - close to the size of our solar system!! Galactic Nucleus: Supermassive Black Hole - created during formation of galaxy - from giant regions of compressed gas and dust near the center

Singularity: - can possibly connect to another spacetime - Einstein-Rosen bridge or "wormhole"