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Boom! • Within 0.25s core is neutrons with radius 20 km and super- nuclear density • Very little light can escape, energy carried off by neutrinos. Power emitted in these exceeds all known stars for 10 s • At this density core collapse stops with bounce • Colliding with infalling layers this triggers shock wave blowing outer star into space (96% of mass for star) • In compressed heated shock wave fusion to Fe and beyond via r- process • As ejecta thin light can escape. Luminosity reaches • Energy released type-II supernova gravitational in origin 1
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Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

Dec 16, 2015

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Page 1: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

1

Boom!• Within 0.25s core is neutrons with radius 20 km and super-nuclear

density• Very little light can escape, energy carried off by neutrinos. Power

emitted in these exceeds all known stars for 10 s• At this density core collapse stops with bounce• Colliding with infalling layers this triggers shock wave blowing outer star

into space (96% of mass for star)• In compressed heated shock wave fusion to Fe and beyond via r-process• As ejecta thin light can escape. Luminosity reaches• Energy released type-II supernova – gravitational in origin

Page 2: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

2

Seeing Them• Sung dynasty history describes a

supernova in 1054 whose remnant – Crab nebula in Taurus – is still visible (M1)

• Japanese, Arabic, Native American records concur

• Milky Way supernovae also in 1006, 1572, 1604. Estimated every 300 years but obscured by dust

• Many visible in other galaxies, currently some 20-30 bright ones

Page 3: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

3

SN 2011dh

Page 4: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Classification• SN classified by spectrum:

– Ia: Strong Si no H He– Ib: Weak H Strong He– Ic: Weak Si no H He– II: Strong H

• Ia are nuclear explosion of WD• II Ib Ic are gravitational core

collapse with degrees of envelope loss

Page 5: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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• 168,000 years ago a B3 I supergiant collapsed in LMC

• Observed as SN 1987A• Progenitor known –

changed theory• Remnants observed in

detail

Page 6: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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The Nebula

Page 7: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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What we are Seeing

Page 8: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Neutrinos• Three hours before the supernova

detected, neutrino detectors observed a burst (20) of neutrinos from the right direction.

• 20 detected implies 1058 emitted carrying 1046 J in agreement with models

• Neutrinos get out before shock wave disperses outer layers, so got here before the light

• Neutrino Astronomy launched, many new experiments planned

Page 9: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

9

What is Left of Core?• Electron degeneracy

cannot stop collapse – few electrons

• Neutron degeneracy pressure at density

• in • Surface gravity

• Physics is relativistic• Chandrasekhar Limit

depends on rotation

• Rapid Rotation expected• High magnetic field frozen

in

Page 10: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Discovery• Physics Predictions:– Rapid Rotation

– Intense magnetic field

– High Temperature

• Bell 1967: Periodic 1.337s Radio pulses: LGM?

• Quickly found other sources: natural

• Soon find many pulsars

Slow down in

Page 11: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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LGM Data

Page 12: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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What are Pulsars?• Rotating star breaks up

• Only NS dense enough to survive

• Emission aligned to magnetic axis - tilted

• Crab pulsar :Neutron star SN remnant

Page 13: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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How They Work• General Idea: Rapidly changing intense

magnetic field creates intense electric field

• Lifts charged particles from polar regions into magnetosphere dragged around by rotation

• Accelerated to relativistic speeds – emit synchrotron radiation at all wavelengths in direction of magnetic axis

• Emitted energy slows rotation• Luminosity of Crab nebula agrees with

observed rate of slowing of pulsar

• Pulsars observed in all bands

Page 14: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Principle of Relativity• Laws of Physics are the same measured at rest

or moving at constant velocity• determines accelerations which are

the same in both frames • At rest is meaningless. Only relative velocities

are physical

Page 15: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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This Week• Follow Principle of Relativity as far as it takes us• Electromagnetism will force some modifications –

Special Relativity• Find that Newtonian gravity is not invariant after all• Describe General Relativity and some Astronomically

important consequences• Black Holes

Page 16: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Space and Time• Space: All possible positions• Motion described by• Plot on three axes to produce worldline• Spacetime: All possible events• Newton I: Objects upon which no forces act

have straight worldlines

Page 17: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Spacetime• Velocity is

slope of worldline from axis

• Stationary objects have vertical worldlines

• Horizontal line (space) is Universe at some time

Page 18: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Relativity in Spacetime• O’ moves at relative to

O• Describe same event by

different coordinates

Page 19: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Velocity Addition

Page 20: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Maxwell’s Problem• Maxwell’s equations predict the speed of

electromagnetic waves in terms of measured properties of electric and magnetic interactions

• Electromagnetism is not invariant under Galilean relativity

Page 21: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Two Possible Solutions• Light propagates at

through aether • Maxwell’s equations

hold for observers at rest relative to aether

• Moving at measure

• Light propagates at through space

• Maxwell’s equations hold for all inertial observers

• Moving at measure

Page 22: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Looking for the Aether• A light clock is two

mirrors at distance• Light bounces between

them in time• Moving light clock

relative to aether will change its rate

Page 23: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Two Motions• Moving along axis • Moving transversely

Page 24: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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The Answer• Michelson-Morley 1887:• Viscous aether dragged by Earth?• Einstein 1905: No Aether. Maxwell’s equations

hold in any inertial frame• Galilean relativity is wrong.

Page 25: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Lorentz Transformations• Send a light pulse from

• Seek

Page 26: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Lorentz Transformations

Page 27: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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The Answer

• For and not too large,

Page 28: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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The Answer

• Note or else this makes no sense

Page 29: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Simultaneity• Most unintuitive:

Simultaneity is Relative• Is causality lost?• Source of many

“paradoxes” Measure distance in light-seconds or time in light-meters so

Page 30: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Time and Simultaneity• Since we know is

constant we can measure time of distant events

• If light from reaches 0 at time it was emitted at

• The present: Events from which light will reach us at

Page 31: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Length Contraction• A ruler lies at

• This is

Page 32: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Time Dilation• Clock at ticks at

Page 33: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Doppler• Doppler formula modified by time dilation

– Transverse Doppler effect

– Longitudinal Doppler effect

Page 34: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Is This Real?• We have lots of experimental evidence • This is real. Any ruler constructed using

Lorentz-invariant physics will contract at high speed. Any physical clock will run slow at high speed

Page 35: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Velocity Addition

Page 36: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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The Invariant Interval• Lorentz transformations

have the property that

lightcone

Page 37: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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What It Means• If an

observer with gets to

• is proper time• If observer

comes from• This is future/past

past

future

Page 38: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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What it Means• If observer with finds is proper distance• Faster observer has order

reversed• Causal theory means no

material particle or information can propagate faster than

past

future

Page 39: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Conservation Laws• Newtonian conservation laws are not Lorentz-

invariant• Find relativistic conserved quantities

Page 40: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Remarks• invariant mass• transform under Lorentz like • These conservation laws hold always. Lavoisier 1777

would find that energy lost to radiation reduced mass slightly

• Decay of a particle that does not conserve mass is consistent with these – and happens

• Other conserved quantities are invariant

Page 41: Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.

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Relativistic Laws• Electromagnetism (Maxwell) is Lorentz-invariant• Nuclear interactions have Lorentz-invariant form• Quantum relativistic version (Quantum Field

Theory 1940/1972.• Gravity????