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Evolution of the Universe from 13 to 4 Billion Years Ago

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    Evolution of the Universe from 13 to 4 Billion Years Ago



    Evolution of the Universe from 13 to 4 Billion Years Ago - Transcript


    Evolution of the Universe from 13 to 4 Billion Years Ago
    Prof Dr Harold Geller hgeller gmu edu http physics gmu edu hgeller Department of Physics and Astronomy George Mason University

    Unity in the Whole Structure
    How is it possible by any methods of observation yet known to the astronomer to learn anything about the universe as a whole It is possible only because the universe vast though it is shows certain characteristics of a unified and bounded whole science shows unity in the whole structure and diversity only in details
    Simon Newcomb 1906

    What I m Going to Talk About
    The Big Bang Theory of the Formation of the Universe
    Radiation Matter and the Physical Laws
    Kirchoff s Spectroscopic Laws Planck s Radiation Curves Stefan Boltzmann Law Newton s Law of Motion Maxwell s Equations for Electromagnetism Hubble s Law Einstein s General Theory of Relativity Bohr s Atom Wien s Law Kepler s Laws of Planetary Motion Newton s Law of Universal Gravitation Doppler Effect Einstein s Special Theory of Relativity Gamow s Big Bang

    The Formation of Galaxies and Stars The Nebular Condensation Theory and the Formation of the Solar System The Formation of the Earth The Precursors of the Formation of Life

    The Big Bang Begats
    Macrocosmos Quantum Fluctuation Radiation Electron Positron Higgs Fields Inflation Cosmos Universe Strong Force Proton Nuclear Fusion Beta Radioactivity Gas Electric Charge Rocks Life Field Cosmic Background Radiation Particles Particle Anti particle Interactions False Vacuum Spontaneous Symmetry Breaking Big Bang Quarks Neutron Alpha Radioactivity Atom Gravity Magnetism Air Humans

    Some Basic Physics
    Kirchoff s Spectral Laws
    Continuous Spectrum
    any body ideal blackbody that is at a temperature above 0 K

    Emission Spectrum
    any low pressure gas that you place a high voltage across

    Absorption Spectrum
    any low pressure gas placed between a blackbody and the observer

    Bohr s Atom
    Best described the workings of the Hydrogen atom
    one proton and one electron around the proton moving in orbits that are discretized quantized so that no intermediate orbits are allowed
    Absorption Emission

    Planck s Radiation Curves
    A way to depict frequency inverse of wavelength versus intensity

    Intensity

    Frequency

    Wien s Law
    Peak wavelength is inversely proportional to the temperature of the blackbody

    Cooler Body
    Peak Wavelength

    Hotter Body Intensity Frequency

    Stefan Boltzmann Law
    Energy radiated by blackbody is proportional to the temperature to the 4th power

    E eg v T me tue n r y s e p ra r
    600 00

    500 00

    Energy

    E

    4 T

    400 00

    300 00

    200 00

    100 00

    0 0 2 4 6 8 1 0 1 2 1 4 1 6

    T me tue e p ra r

    Kepler s Laws
    Kepler s First Law of Planetary Motion
    planets orbit sun in an ellipse with sun at one focus

    Kepler s Second Law of Planetary Motion
    planets sweep out equal areas in equal times
    travel faster when closer slower when farther

    Kepler s Third Law of Planetary Motion
    orbital period squared is proportional to semimajor axis cubed P2 a3

    Newton s Laws I
    Newton s First Law of Motion
    body at rest tends to stay at rest and body in uniform motion will stay in straight line uniform motion unless acted upon by an outside force

    Newton s Second Law of Motion
    the acceleration of a body is proportional to the force being applied

    F ma

    Newton s Laws II
    Newton s Third Law of Motion
    for every force there is an equal and opposite force action and reaction

    Newton s Law of Gravitational Attraction
    force is proportional to masses and inversely proportional to the distance squared

    F G m M r2

    Doppler Shift
    A change in measured frequency caused by the motion of the observer or the source
    classical example of pitch of train coming towards you and moving away

    Maxwell s Electromagnetism
    Electricity according to Gauss
    relates electricity to electric charge

    Faraday s Law
    relates electric fields to magnetic fields

    Magnetism according to Gauss
    relates magnetism to electricity

    Ampere Maxwell Law
    relates magnetic field to electricity

    Einstein s Relativity Theories
    Special Theory of Relativity
    speed of light constant in all reference frames
    time dilation and simultaneity length and mass addition of velocities

    General Theory of Relativity
    Principle of Equivalence curvature of space time

    Hubble s Law
    The further away a galaxy is the greater its recessional velocity and the greater its spectral red shift

    v H0d
    There is a simple linear relationship between the distance a galaxy is from the Earth and the redshift of that galaxy which is a measure of the speed with which a galaxy is moving away from the Earth

    The value of the Hubble constant H0 is not known with certainty but best value today is approximately 67 km s Mpc

    Hubble s Conculsion
    From Hubble s Law we can calculate a time in the past when universe was a point Big bang occurred about 13 15 billion years ago
    big bang formally proposed by Gamow based upon such evidence
    Big bang theory progenitors existed in looser manner

    Gamow s Big Bang and Hoyle s Steady State
    Steady State Universe
    universe looks same and will look same
    continuous creation

    Big Bang Universe
    universe began in big bang or ylem
    single point of creation

    In The Beginning
    In the beginning God created the particles and the antiparticles Now the temperature was high and the particles and the antiparticles were in equilibrium And God said Let there be light and He separated the photons from the particles and antiparticles God called the photons bosons and the particles and antiparticles He called fermions And there was pair production and there was photon creation the first 10 43 seconds
    Eric Schulman from A Briefer History of Time

    Details of the Big Bang
    The littlest of physics The Big Bang ensuing Cosmic Eras
    The Vacuum Era
    The Planck Epoch and The Inflationary Epoch

    The Radiation Era
    Light and Baryons The Electroweak Epoch and The Strong Epoch Decoupling and the creation of matter

    The Matter Era
    Transition to matter Galaxy Formation Epoch and Stellar Epoch

    The Degenerate Dark Era
    Dead Star Epoch and Black Hole Epoch

    Whither the future

    The Littlest of Physics
    Space Time Matter and Forces Types of Matter
    Quarks Baryons
    protons neutrons

    Electrons Leptons
    electrons neutrinos muons

    Types of Forces
    gravity electromagnetism strong weak

    Back to the Beginning
    The universe began as an infinitely dense cosmic singularity which began its expansion in the event called the Big Bang which can be described as the beginning of time During the first 10 43 second after the Big Bang the universe was too dense to be described by the known laws of physics

    The Vacuum Era
    The Planck Epoch
    10 43 sec and about 1019 GeV 1 GeV 1013K we just don t know

    The Inflationary Epoch
    10 43 sec 10 10 sec expansion driven by repulsive gravity

    Inflation was one of several profound changes that occurred in the very early universe

    Four basic forces explain all the interactions observed in the universe

    Grand unified theories GUTs are attempts to explain three of the forces in terms of a single consistent set of physical laws A supergrand unified theory would explain all four forces GUTs suggest that all four physical forces were equivalent just after the Big Bang

    The Radiation Era
    Creation of light Creation of baryonic matter Electroweak epoch Strong epoch Decoupling of weak interaction Creation of nuclei of the light elements Decoupling of radiation spectrum

    When the temperature of the radiation fell below 3000 K protons and electrons could combine to form hydrogen atoms and the universe became transparent

    The Matter Era
    Transition from radiation domination to matter domination Last scattering Dark Ages Galaxy Formation Epoch Bright Ages

    The Degenerate Dark Era
    Whither the future
    death of stars black hole domination What will happen to the remaining matter in the universe
    Ultimately sucked into black holes Ultimately all black holes combine Ultimately all spit out in a new big bang

    Summary Timescale
    Era The Vacuum Era Epochs Main Event Time after bang 10 43 sec 10 10 sec 10 10 sec 10 4 sec 1 sec 1 month 1 2 billion years 2 15 billion years 20 100 billion yrs 100 billion Planck Epoch Quantum Inflationary Epoch fluctuation Inflation

    The Radiation Era Electroweak Epoch Formation of Strong Epoch leptons bosons Decoupling hydrogen helium and deuterium The Matter Era Galaxy Epoch Galaxy formation Stellar Epoch Stellar birth The Degenerate Dark Era Dead Star Epoch Black Hole Epoch Death of stars Black holes engulf

    A Thoughtful Break
    The grand aim of all science is to cover the greatest number of empirical facts by logical deduction from the smallest number of hypotheses or axioms
    Albert Einstein 1950

    The Evidence So Far
    Evidence for a Big Bang
    expansion of the universe
    galaxies receding from us
    everywhere the same

    remnants of the energy from the Big Bang
    a very hot body that has cooled
    2 7 K cosmic background radiation

    the primordial abundance of chemical elements

    What CMB means
    Cosmic Microwave Background
    Remember Wien s Law Remember Doppler COBE results

    Cosmic Background
    How hot would the cosmic background radiation be
    close to 3 K
    first detected by Penzias and Wilson of Bell Labs
    Didn t know what it was Explained by Robert Dicke of Princeton Didn t get a piece of the Nobel Prize with Penzias and Wilson

    confirmed by COBE satellite

    Putting it into context
    Taking the perspective of the universe with you at the center

    The CMB remainder
    Using COBE DIRBE data for examining the fine differences
    fine structure of the universe
    led to the galaxies and their location

    Astronomers use supercomputers to simulate how the large scale structure of the universe arose from primordial density fluctuations

    Linking the CMB to the Galaxies

    Galaxies are grouped into clusters rather than being scattered randomly throughout the universe

    String Theories Attempt to Unify Physical Forces
    The search for a theory that unifies gravity with the other physical forces suggests that the universe actually has 11 dimensions ten of space and one of time seven of which are folded on themselves so that we cannot see them The idea of higher dimensions has motivated alternative cosmological models No evidence to support string theories at this time

    What I Talked About
    The Big Bang and Everything Within The Evidence for the Big Bang
    Hubble s Law Cosmic Microwave Background Abundance of chemical elements

    A touch of strings