Monday, September 17 Thorne pgs.: 104—End of Ch. 5.

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Presentation transcript:

Monday, September 17 Thorne pgs.: 104—End of Ch. 5

Agenda Announce: Read up to Ch. 9 by next week Review Last week Tides

Review Reference Frames Einstein’s Special Theory of Relativity What’s relative/absolute? Effects Einstein’s General Theory of Relativity Equivalence principle Emerging Picture of Einstein Non-conformist Does what he likes (“lazy dog”) Worked mostly in isolation (unusual) Guided by aesthetics Used thought (gedankin) experiments

Tides What produces tides on Earth? Why were tides important for moving beyond the equivalence principle?

Curvature Spacetime curvature the same thing as Newton’s tidal gravity Objects move in geodesics Viewing curvature…embedding in a flat space (fig. 3.3 on page 129)

The Math Einstein got help from friend Marcel Grossman Studied Riemannian geometry What did they seek? How did Einstein know if he had found it?

The solution Needed a formula that gave the curvature Kept having problems finding one that gave the same answer in all frames Eventually found one that also gave a good number for the precession of Mercury’s orbit

Newton’s Black Holes What’s a dark star?

Schwarzschild And let there be relativists…within a year Schwarzschild found important “solution” Dead four months later Described curvature of spacetime in vicinity of spherical star More massive or compact a star was, the more the effects: Gravitational redshift and time dilation near surface Couldn’t continue forever for the most massive of stars…

The Prediction of Black Holes Einstein rejected them Claimed that as a star shrunk, particles would have to move faster than light to maintain pressure

Massive Stars: White Dwarfs Very dense Most stars demonstrate a balance: Thermal pressure Gravitational squeezing What forces can balance gravity at extremes?

The Search for Forces Chandrasekhar to the rescue Use of quantum mechanics Electron degeneracy pressure Monstrous densities mean high speeds for trapped particles Particle’s now have max speed, hence density limit White dwarfs can’t be heavier than 1.4 Suns! What happens to such stars?

Zwicky Supernova Neutrons Neutron stars