general theory of relativity secs 29.1-29.3 professor ken wester

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General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

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Page 1: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

General Theory of Relativity

Secs 29.1-29.3

Professor Ken Wester

Page 2: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

Reminders 1

• Lab this week due by Friday at 4:00 pm: B1-WA: Wave Addition

• Weekly Reflection #11 due by late tonight• Weekly Reflection #12 (due 11/11) was sent

out last week.• Reading quiz due prior to the start of class on

Thursday (Chap 29, Sec 4) – now available.• In-class Quiz #5 (Chapters 11-13) today

Page 3: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

Reminders 2

• Test #3 (Chapters 8, 9, 11-13) on Tuesday, November 11th (29?@1pt, 1?@2pts) Max score = 120%; Test starts at 8:15 AM. Mostly qualitative.

• No class on Thursday, November 13th

• In-class Quiz #6 moved to Thurs, November 20th

• When in doubt, consult the syllabus.

Page 4: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

‘Boundaries” in Physics

• Today we start to cross a second threshold between three types of physics (common to all sciences):– Observational– Experimental– Theoretical

• Each of the above relies upon the others, and none stands entirely on its own.

Page 5: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

Albert Einstein

• Albert Einstein (3/14/79 - 4/18/55, b. in Ulm, Germany) developed special (1905) and general (1916) theories of relativity.

• The most influential physicist of the 20th century – if not all time .

• Revolutionized physics yet a third time (after Newton and Maxwell)

Page 6: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

Einstein

• Best known for E=mc2

• 1905 Annus Mirabilis:– Brownian motion– Special relativity– Photoelectric effect

• His 1905 paper “On the Electrodynamics of Moving Bodies” was the birth and source of Special relativity.

• In this article he noted that Newtonian mechanics could not be reconciled with Maxwell’s work.

• Received the 1921 Nobel Prize in Physics for the photoelectric effect.

• Established the basis for quantum mechanics.

Page 7: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

Einstein

• He realized after creating Special Relativity that the principle of equivalence could also be extended to gravitational fields.

• He published his General Theory of Relativity in 1916.

Page 8: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

Equivalence Principle 1

• Based on the question, “What happens if a reference frame accelerates?”– Weightlessness depends on the frame of

reference such as with a falling elevator or a spaceship in orbit around Earth.

– Artificial “gravity” occurs in a rocket or spinning spacecraft because of Newton’s first law of motion.

– This artificial “gravity” cause by acceleration cannot be distinguished from gravity caused by the presence of matter.

Page 9: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

Equivalence Principle 2

• Inertial frames of reference are those in which Newton’s laws of motion apply.– All small freely falling reference frames are inertial

(Newton’s 1st law holds – no fictitious forces).– A small, uniformly accelerated reference frame is

indistinguishable from a reference frame in which there exists a gravitational field.

• To create an (artificial) gravitational acceleration (or force) in a given direction in a reference frame, accelerate the frame in the opposite direction.

Page 10: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

Consequences of Equivalence Principle

• Prediction: Deflection of Light’s Path– An apple thrown or light beam shot across the short

axis of accelerating rocket is deflected.• Prediction: Gravitational Doppler Shift– When moving against a gravitational field, light loses

energy (E = hc/λ) while speed remains constant.• Prediction: Gravitational Time Dilation– Note that λ/T = c. (Recall that λf=c and f=1/T). If λ

increases, then T increases. Gravity slows clocks.

Page 11: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

First Experimental Verification

• In 1919, Einstein’s prediction of the bending of starlight were verified during a total solar eclipse by Sir Arthur Eddington.

Page 12: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

Consequences of Matter’s Presence

• Gravity distorts space, introducing fictitious forces – two apples following to Earth center.

• Gravity distorts space changing world lines.– Flat space– Positively curved space– Negatively curved space

• Curved space has “higher dimensionality” – consider Edwin Abbott’s Flatland

Page 13: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

Consequences of Space Curvature

• Flat or zero curvature:– Triangles = 180 degrees; parallel lines are parallel; one

can travel in a straight line indefinitely, space unbounded• Positive curvature:

– Triangles > 180 degrees, “parallel” lines converge, travel in a straight line and end up at start, space bounded

• Negative curvature:– Triangles < 180 degrees, “parallel” lines diverge, travel in

a straight line indefinitely, space unbounded• “Miracles” become understandable (Abbott)

Page 14: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

Experimental Tests of GTR

• Precession of the perihelion of Mercury– Explained that not explained by classical mechanics

• Deflection of star light– Verified in 1919 solar eclipse

• Gravitational reddening of Sirius B– Verified by spectral studies of the white dwarf star

• Gravitational waves– Verified using binary pulsar and decay of period

• Global positioning systems– GTR corrections required for onboard orbiting clocks

Page 15: General Theory of Relativity Secs 29.1-29.3 Professor Ken Wester

The Two Theories of Relativity

Special Theory (1905)• Based on the question,

“What would the world look like if I rode on a beam of light?”

General Theory (1916)• Based on the question,

“How does the presence of matter affect space?”