history of science (part ii)€¦  · web viewphase transition from false vacuum state (guth 1981)...

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History of Science (Part II) :Cosmology Recall: Galileo Telescopic observation Moons of Jupiter Phases of Venus Sunspots Promoted Copernicus Censored Defended Copernican system Dialogue of the Two World Ssytems Tried by the Inquisition (1633) Discourse on Two New Sciences (1637) : kinematics No treatment of causes of motion 1

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Page 1: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

History of Science (Part II) :Cosmology

Recall: Galileo

Telescopic observation

Moons of JupiterPhases of VenusSunspots

Promoted CopernicusCensored

Defended Copernican system Dialogue of the Two World Ssytems

Tried by the Inquisition (1633)

Discourse on Two New Sciences (1637): kinematicsNo treatment of causes of motion

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Page 2: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Recall:

Newton: Principia (1687)

Law 1 Every body continues in its state of rest, or uniform motion in a straight line, unless compelled to change by forces acting on it

Law 2: The change in motion is proportional to the force impressed, and in the direction of the force

Law 3: To every action there is always an equal and opposite reaction: the mutual actions of two bodies upon each other are always equal, and directed to contrary parts

Summ: N2

F = force actingF = ma m = mass

a = accel

Notes1. force causes accel (F = 0 ↔ a = 0)2. accel is proportional to force acting3. accel is inversely proportional to mass of object4. inertial mass is constant

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Page 3: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Law 4: Universal Law of Gravitation

FG = GMm/r2

FG = force of gravity M = mass of one object

m = mass of other object r = separation of objects

G = constant (6.6x 10-11)

Unites terrestrial and celestial gravityForce on apple = force on planets

Notes:

1. FG v. weak force (G extremely small)FG only seen when one mass is a planet

2. FG always attractive3. FG acts instantaneously across huge distances 4. M,m = inertial mass (see N2)

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Page 4: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Newton’s Cosmos

1. Force of gravity – Attractive, weak, infinite range

2. Univ. infinite in time (eternal)no beginning, no end

3. Univ. finite in contentGravity would crush universeOlber’s paradox

4. Space – infinite?Space and time a fixed stage

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Page 5: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

19th century cosmology

1. Improved telescopes Distances to stars

2. Photography Improved images

3. SpectroscopyAnalysis of starlightSpectral lines of known elements

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Page 6: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

The Great Debate 1900-1920

1. Detection of the distant nebulae

2. Stars within Milky Way ? (Shapley)Measured diameter of Milky way – enormous

3. Galaxies outside Milky Way ? ( Curtis )Motion too great to be confined to Milky wayEmission lines doppler-shifted : Vesto Slipher

4. Measurement of distance to nebulae (Hubble, 1925)Cepheid variables

Much larger than diameter of Milky Way

Conclude: many distant galaxies !

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Page 7: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Hubble’s Law

1. Detected galaxies outside Milky WayCepheid variables

2. Combined with velocity measures of nebulae (galaxies)

Vesto Slipher

3. Relation between distance and velocity of a galaxy

Hubble’s Law v = Hod (1929)

Linear relation Ho = slope = measure of expansion rate

uncertain due to distance calc

4. Hubble’s Law II (1931)

more accuratemeasurements of distance to 40 galaxies – Hubblemeasurement of 40 redshifts – Humason (assistant)

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Page 8: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

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Page 9: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

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Page 10: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Albert Einstein (1867-1955)

Special Relativity (1905): breakdown of Newtonian mechanics at high velocities

Speed of light universal constDistance, time and mass velocity-dependent!Space-timeMass-energy (E = mc2)

General Relativity (1915) : breakdown of Newtonian mechanics at high gravitational fields

Gμν = -kTμν (10 eqs)

Geometry of space-time (Gμν) is determined by distribution of matter and energy (Tμν)

“Gravity = distortion of space-time by mass”

Relates geometric properties of space-time

(curvature and expansion) to

properties of matter (density and state of motion)

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Page 11: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

GR and cosmology

Note: 10 equations of GR : solutions?

Note: Assume Cosmological Principle:U is homogeneousU is isotropic

Note : Solutions of GR equations are dynamic (U expanding or contracting)

Solutions: Einstein, deSitter, Friedmann, Lemaitre

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Page 12: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

1. Einstein’s cosmology

Believed U static, unchanging

Introduced cosmological constant λ for static U

Gμν + λgμν = -kTμν

Note: Failed to predict expanding U

Greatest blunder

Rejected Friedmann solns

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Page 13: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

2. Alexander Friedmann

Solns of GR (1922) assuming Cosmological Principle

No cosmological constant: space-time dynamic

Expanding U: balloon model

Density of matter = clock

Friedmann Models

Closed U: gravity > expansion (+ve curvature)Open U: gravity < expansion (-ve curvature)Flat U : gravity = expansion (flat U)

1. Def: critical density of matter dc

If density of U > dc → U eventually collapseIf density of U < dc → U expand forever

2. Define Ω = d/dc

Ω > 1 → U eventually collapseΩ < 1 → U expandΩ = 1 → Dividing line

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Page 14: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

3. Georges Lemaitre

Mathematician and physicist (Louvain)Astronomy at Cambridge, Harvard and MIT

1. Solns of GR (1922) assuming Cosmological Principle

No cosmological constant: space-time dynamicExpanding U: balloon modelIndependent of Friedmann

Three Models Closed U: gravity > expansion (+ve curvature)Open U: gravity < expansion (-ve curvature)Flat U : gravity = expansion (flat U)

2. Compares to astronomical measurements Dynamic U and Slipher redshifts Obscure journal(1927)

3. Shows to Einstein (1927) Rejected Referred to Friedmann’s work

4. Republished in 1931 (Eddington) Hubble’s law causes Eddington rethinkRedshift section missing?

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Page 15: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Hubble’s Law and relativity

Linear relation between distance and velocity of a galaxy

Red-shifted galaxies: receding sourceCoverted redshift to recession velocity v

Hubble’s Law v = Hod (1929)

Ho = slope = measure of expansion rate, of K.E.- difficult to measure due to distance calc

Hubble’s Law II (1931) Measurements of distance to 40 galaxies – Hubble Measurement of 40 redshifts – Humason (assistant)

Hubble’s Law and relativity Einstein accepts dynamic universe (1931)

Eddington, Einstein consider new universeLemaitre paper republished (1931)Lemaitre/Friedmann model accepted

Note: redshift due to stretching of space-time (expansion)

Note: gravity prevents expansion locally

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Page 16: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Origin of the Universe: Lemaitre

Lemaitre (1931): Rewind expansion: U once extremely small? Cataclysmic origin to U?

Mechanism (1931): Primeaval atomProcess of radioactive decay

Problem: Hubble age ~ 2 billion yr (faulty Ho)

Conflict with age of stars: ~ 10 billion yr

Lemaitre: re-introduce cosmological constant?

Reception: not popularAge paradox a major problem

Primeval atom rejectedOrigin theory rejected

(Note: Ho later revised, age problem disappears)

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Page 17: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Origin of the Universe: Gamow

Gamow: Trained under Friedmann (relativity)Expert in nuclear physics

Research: Nucleosynthesis of the elements nuclear fusion in the stars

Problem: Theory cannot explain abundance of the lightest elements

Gamow (1940s): Relativity predicts infant universe extremely dense, hot

Synthesis of the elements in the infant universe?

1942: Recruits Ralph Alpher to work it out (YLEM)1948 : Alper, Bethe, Gamow paper

Hydrogen (75%), helium (25%)

Success: in agreement with observation 2nd plank of evidence for BB

Snag: fails to explain formation of the heavier elements

Note: now known that heavier elements are formed in stars and supernovae

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Page 18: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Origins: a third prediction

Gamow et al: synthesis of the light elements in infant U

Alpher and Herman: early u dominated by hot radiation

radiation present in today’s universe?

Recombination: as universe expands, it cools particles coalesce into atomsscattering of radiation reducedU becomes transparent to radiation

Radiation left over from time of recombination?(200,000 yr after bang)

Extremely low temperatureRed-shifted

Alpher and Herman (1948): radiation should remain as cosmic backgound field

Temp ~ 5 KelvinFrequency: microwaves

Reception: Gamow group ignoredNo search for radiation

Note: CMB discovered accidently in 1965

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Page 19: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Steady State model of U

Gold, Hoyle, Bondi: Cambridge 1940s, 50s

Unhappy with Lemaitre/Gamow model

1. Age problem2. Singularity problem3. Nucelosynthesis of heavier elements

Film: In the Dead of Night

Gold: could U be dynamic but unchanging?

Expanding but homogenous in time

Perfect Cosmological Principle

Hoyle: continuous creation of matter

Only tiny amount needed

No need for originNo age problemPhysical reason for expansion

New matter making space for itself

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Page 20: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

A Cosmic Debate

U different in the past ? (Big Bang)U same in the past ? (Steady State Model)

Evidence that U was different in the past would rule out Steady-State

Evidence that U was identical in the past would rule out Big Bang

Hoyle: populizer of sciencecoined term Big Bang in derision

Resolution : radio-astronomy

Martin Ryle: Count most distant radio sources

Cambridge radio counts: 1959, 62, 65

Excess of radio sources at the largest distances

Implies

U different in the past

Conclusion: Steady – State model wrong

Bonus: Cosmic background radiation

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Page 21: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Cosmic Background Radiation

Penzias and Wilson (1965): sensitive microwave receiver

Ubiquitous background radiation

Microwave frequency, extremely low temp (3K)

Independent of time, place, orientation of receiver

Impossible to get rid of

Astronomical origin

Explanation: Dicke and Peebles (1965)

CBR Leftover from Big Bang

Correct wavelength, temp

New evidence for Big Bang

Note: Two papers in Astrophysical journal 1965Prediction of Gamow group (1948) ignored at first

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Page 22: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Cosmic background radiation: theory

Radiation produced in early stages of primordial fireballElectrons stripped off atoms – plasma

Up to 100,000 yr after BB: U as hot as the sunphoton scattering by particlesopaque to light

As universe cools:atoms formrecombinationphoton scattering reducedU transparent

Cosmic Microwave Background: relic of radiation at recombinationu.v radiation originallyred-shifted, cooled by U expansion observed at microwave frequenciesextremely low temperature

Note: major new plank of evidence for BB major area of study in modern cosmology

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Page 23: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Evidence for Big Bang (1970s)

1.Hubble’s LawExpansion of U

2. Stellar compositionNucleosynthesis of the elementsHydrogen and helium proportions

3.Radio countsHigher no. galaxies in the past

4.Cosmic background radiation (1965)Temperature, uniformity, extra-galatic

5. Stellar ageAgrees with revised Hubble constant

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Page 24: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Big bang parameters (1970-)

1. Ho = measure of expansion rate = measure of K.E. of U

2. Ω = measure of density of matter in U Ω = density/critical density

3. Expansion = competition between Ho and Ω

Neither Ho , Ω specified by Friedmann eq

Ho : Astronomical distance measurementsBaade, Sandage, de Vancouleurs, HST;

Ω : Nucleosynthesis

Mass of galaxiesGravitational motionGravitational lensing

Ω ≈ 0.3 ?

Includes dark matter

Dark Matter: gravitational effect due to unseen matter

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Page 25: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Big Bang problems

1. Spacetime singularity at beginning (BH)

- extrapolation of GR to quantum times incorrect?- need quantum gravity

2. Structure problem How did galaxies form?Natural fluctuations in density too small

3. Flatness problem

Ω must ≈ 1 (GR: deviations accelerate - Dicke)Observation : Ω ≈ 0.3

4. Horizon problem Large-scale smoothness of UFaster than light communication?

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Page 27: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Inflation

1. Particle physics and cosmology (1980s)

2. GUT - Monopole problem

3. Phase transition from false vacuum state (Guth 1981)

Hugely accelerated expansion during at start of BBPhase transition accompanied by vacuum energy

Solution for flatness problem

Ω →1

Huge balloon is flat

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Page 28: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Solution for horizon problem

A universe that underwent an exponential expansion will be causally connected

A mechanism for galaxy formation

Could natural inhomogeneities in an inflationary universe give rise to today’s galaxies?

Hawking, Guth, Linde et al: yes

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Page 29: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Inflation - snags

1. End of inflation

2. Prediction of flatness

Ω = 1 ?Conflict with evidence?

3. Inflationary field?Inflationary process?

4. Observable universe

5. Many universes?

Extravagant explanation

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Page 30: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Modern measurements

1. Ripples in microwave background (1992) Fluctuations in density, amplified by gravity

2. Gravity waves (1990s)

shock waves from cataclysmic event-indirect evidence

3. Gravitational lensing (1980s) gravity of galaxy splits light from starrejoins when galaxy pastring of light seenused as lens system in astonomy

4. Acceleration of U (1998)Not predicted by Friedmann (GR)

Soln: new cosmological constant in GR

5. U has flat geometry (2000)Measurements of angular variations of CMB

Ω =1

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Page 31: History of Science (Part II)€¦  · Web viewPhase transition from false vacuum state (Guth 1981) Hugely accelerated expansion during at start of BB. Phase transition accompanied

Acceleration of U

Experimental measurements (1998-)

Not predicted by Friedmann solns (GR)

Suggests: dark energy- new cosmological constant

Most likely: energy density of vacuum = ρ

Gμν + = 8ΠG (Tμν + ρgμν)

predicted by quantum theory

particle-antiparticle creation/annihilationvirtual particles

causes gravity to push instead of pull

could cause flat U with acceleration

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