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The Energy in our Universe Dr. Darrel Smith Department of Physics
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Sources of Energy in the Universe 1. Matter a. Gravity b. Fusion 2.Photons -- CMB 2.7 deg. 3.Neutrinos -- 1.7 deg. 4. Dark Matter 5. Dark Energy
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Our Sun How much power is generated by the sun? a) 200 megawatts2 x 10 8 watts b)5,000 terawatts5 x 10 15 watts c)2,500 exawatts2.5 x 10 21 watts d)380,000,000 exawatts3.8 x 10 26 watts The power is called the Luminosity (watts)
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How does it make that energy? Fusion of hydrogen p p p n e + e T + D He 4 + n Surface Temperature vs. Core Temperature
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What does it cost to make all this sunshine? In other words, what does this do to the mass of the sun? a)Mass is converted to energy b)Power d) 1% of the solar mass 100 billion years to burn off
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Energy from type 1a Supernovae Type 1a Supernovae a)Releases a uniform amount of energy 1-2 x 10 44 joules b)Luminosity~ 5 billion times greater than the sun c)~10 billion stars in our Milky Way galaxy
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Formation of a supernovae
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Remnants of Supernovae Crab Nebula (1054 AD) Power output = 5 x 10 31 W = 130,000 L o A pulsar in the core provides the energy. Pulsar is a highly magnetized rotating neutron star. Rotational K.E. is decreasing.
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Supernovae observed 1054 ADObserved by the Chinese Observed by Anasazis in Chaco Canyon 6500 light years away 1987ASupernova in the Large Magellanic Cloud.
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Supernovae Summary 1. Energy comes from where? 2. Where does the energy go? 3. Source of heavy elements 4. Indicator of Dark Energy
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Particle Astrophysics Big Bang Cosmology How do we know what the early universe was like? The LHC at CERN
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Big Bang Cosmology From t=0 through today How do we know this? Particle Astrophysics
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Particle Astrophysics The Tevatron at Fermilab
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The Large Hadron Collider (LHC) Geneva, Switzerland
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Standard Model The physicists equivalent to the periodic table. Unifies QCD with EW interactions into a single structure. It does not include gravity. It is a quantum field theory that is consistent with quantum mechanics and special relativity.
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Standard Model q = +2/3 e q = -1/3 e q = 0 e q = -1 e
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Particles have masses M p = 0.938 Gev/c 2
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Big Bang Cosmology
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What is the Higgs Particle? So, how do particle acquire mass? Through their interaction with the Higgs field. W+W-ZoW+W-Zo
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How is the Higgs formed? The fusion of one quark from each proton. Coming together at high energy. A simulated event in the Atlas detector
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How is the Higgs formed? The fusion of one gluon from each proton. Coming together at high energy. A simulated event in the Atlas detector
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Why such a big machine? We need high energies to make massive particles. E = mc 2
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Why such small distances? We need to put that energy in a small volume to make a high energy density. = h/p
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Mass vs. Size Mass is not proptional to size. Masses of the W and Z particles M W = 82 GeV/c 2 M z = 90 GeV/c 2 M proton = 0.928 GeV/c 2
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Galactic Rotation Curves Velocity = constant (??) Bulge + Disk + Dark Halo
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Where’s the “missing mass” ? Could it be neutrinos? Could it be black holes?
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Solar Neutrinos What happens to the e ’s ?
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Cosmic Ray induced neutrinos ~one-half of the ’s are disappearing in the atmospheric neutrinos Atmospheric Neutrinos ’s ??
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Black Holes Galaxies with Active Galactic Nuclei Schwarzchild Radius Newtonian Mechanics Dump mass on the earth
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Do we see enough dark matter? No !! We can only account for 5-10% of the observed dark matter in the universe What about other sources? MaCHO’sWIMP’s Black Holes and ’s
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Dark Energy Different from “dark matter” It causes the universe to expand (i.e., to accelerate outward. How is this observed? http://imagine.gsfc.nasa.gov/docs/science/mysteries_ l1/dark_energy.html http://imagine.gsfc.nasa.gov/docs/science/mysteries_ l1/dark_energy.html
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Dark Energy Changes in the rate of expansion The more shallow the curve, the faster the rate of expansion.
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Dark Energy Most of the energy in the universe today is “dark energy.” Next, comes “dark matter.” Only 4% of the universe is made of “regular matter.” Neutrons, Protons, electrons, photons, & neutrinos.
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Exotic Propulsion How can we travel through our galaxy? Matter-Antimatter propulsion Nuclear-Thermal Propulsion Faster-than-light propulsion (??)
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