The Music of the Spheres -- symmetry and symmetry breaking in Nature -- Stephen Lars Olsen Seoul National University
Johannes Kepler [ ]
Symmetry & Beauty
Hokusai views of Fuji View 18View 20
Hiroshige views of Fuji View 4View 14
Temple of heaven (Beijing)
From a different angle
Seoul Arts Center 만화경
Snowflakes 60 0
Kaleidoscope 만화경
How it works rotate by 45 0 Start with a random pattern Use mirrors to repeat it over & over The attraction is all in the symmetry Include a reflection
Rotational symmetry No matter which way I turn a perfect sphere It looks identical
Space translation symmetry Mid-west corn field
Time- translation symmetry in music repeat repeat again & again
Prior to Kepler, Galileo, etc God is perfect, therefore nature must be perfectly symmetric: Planetary orbits must be perfect circles Celestial objects must be perfect spheres
Tycho Brahe [ ]
"Music of the Spheres" by Michail Spiridonov
Seoul Arts Center
Kepler: planetary orbits are ellipses; not perfect circles Kepler’s 1 st law: published in July 1609 (500 years ago)
Galileo & his telescope 1 st recorded observations were in July 1609 (500 years ago) Discoveries: Moons of Jupiter Saturn’s rings Phases of Venus and…
1 st seen January 7, 1610 Galileo’s sketches of the Moon’s changing locations Moons of Jupiter
Rings of saturn Sketch of Saturn by Galileo in 1616
Clear evidence that Venus orbits the Sun (& not the Earth) Galileo's sketch of the phases on Venus Phases of Venus Modern photos of Venus
& mountains on the Moon
Modern photo of the Moon The Moon is not a perfect sphere
Symmetries of the laws of Nature
Newton’s laws implicitly assume that they are valid for all times in the past, present & future Processes that we see occurring in these distant Galaxies actually happened billions of years ago Newton’s laws have time-translation symmetry
The Bible agrees that nature is time-translation symmetric The thing that hath been, it is that which shall be; and that which is done is that which shall be done: and there is no new thing under the sun Ecclesiates 1.9 이미 있던 것이 후에 다시 있겠고 이미 한 일을 후에 다시 할지라 해 아래 는새 것이 없나니 전도서 1.9
Newton believed that his laws apply equally well everywhere in the Universe Newton realized that the same laws that cause apples to fall from trees here on Earth, apply to planets billions of miles away from Earth. Newton’s laws have space-translation symmetry
rotational symmetry F F a a F = m aF = m a Same rule for all directions (no “preferred” directions in space.) Newton’s laws have rotation symmetry
Symmetry recovered Symmetry resides in the laws of nature, not necessarily in the solutions to these laws.
Conservation Laws
Conservation of Momentum Momentum= mass x velocity total momentum before = total momentum after
Finding nemo eating
Concept of Kinetic Energy Emilie du Châtelet ( ) Brilliant mathematician One of Voltaire’s lovers K.E.= ½ MV 2
Conservation of energy h max E tot =mgh max E tot =1/2 m(v max ) 2 Total energy = Kinetic Energy + Potential Energy + Heat Energy = Constant
Energy conversion of a skier Friction: energy gets converted to heat Potential energy Potential energy kinetic energy Total energy = Kinetic Energy + Potential Energy + Heat Energy = Constant
Conservation of angular momentum
Emmy Noether Conserved quantities: stay the same throughout a process Symmetry: something that stays the same throughout a process Conservation laws are consequences of symmetries
Symmetries Conservation laws Symmetry Conservation law Rotation Angular momentum Space translation Momentum Time translation Energy
Atomic spectra
Decoding atomic spectra Mercury spectrum Mercury energy levels “quantum jump”
Laporte Rule even odd even oddeven odd even odd even X X
Even & Odd functions L R R L Even Function Odd Function Does not change Changes sign Parity = +1Parity = -1