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The Lyman Alpha Forest

The Lyman Alpha Forest. By Shira Mitchell. Ionized universe. Neutral universe. Star Formation. Big Bang. When did stars form?. Wavelength. What is a Spectrum?. The distribution of energy emitted by a radiant source. Intensity. Wavelength. Electron excited. Photon 1216 A. Atoms.

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The Lyman Alpha Forest

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  1. The Lyman Alpha Forest By Shira Mitchell

  2. Ionized universe Neutral universe Star Formation Big Bang

  3. When did stars form?

  4. Wavelength

  5. What is a Spectrum? The distribution of energy emitted by a radiant source Intensity Wavelength

  6. Electron excited Photon 1216 A Atoms n=4 n=3 n=2 n=1 Hydrogen Atom Energy Levels

  7. Electron excited Atoms n=4 n=3 n=2 n=1 Hydrogen Atom Energy Levels

  8. Absorption Intensity Wavelength Wavelength Wavelength

  9. Redshift z = Observed wavelength - Rest wavelength Rest wavelength The Cosmological Redshift is a redshift caused by the expansion of space.

  10. Hubble’s Law v = H*r. v = recessional velocity r = distance from Earth H = Hubble's constant, 50-100 km/sec/Mpc (a megaparsec is 3,000,000 light-years) Hubble constant sets the rate at which the Universe is expanding.

  11. Redshift • z = 6 farther back to the universe’s beginnings than z = 3 • Astronomers speak of the history of the universe in terms of red-shifts

  12. Quasars Short for quasi-stellar radio sources. They are bright active galaxy nuclei with huge red-shifts and therefore, far distances

  13. Neutral hydrogen absorbed this light Quasar Spectrums Intensity Wavelength

  14. Quasar Spectrums

  15. Why is there a forest? If the universe has so much hydrogen, why is there no trough? The hydrogen must be ionized because ionized hydrogen can not absorb light. Why is the hydrogen ionized? The radiation from stars Therefore, to find the trough, one must look at very very distant quasars to look for the trough back towards the universe’s beginnings.

  16. Looking for the Trough 13 Apr 2000 Using the powerful Keck telescope on Mauna Kea in Hawaii, Robert Becker and his colleagues detected the imprint of neutral atoms on light from quasar J1030 0524, one of the most distant objects yet found. They found that, over a region of the spectrum corresponding to millions of years of cosmic history, no light from the quasar gets through -- it is all absorbed in intergalactic space.

  17. Looking for the Trough

  18. Gun-Peterson Trough Quasar Spectrums z=5.80 z=6.28 z = 6 means it left the sources less than a billion years after the Big Bang

  19. Why is this important? To understand the complex universe we live in today, it is necessary to understand its evolution from an early state of simplicity.

  20. Current Progress • Some astrophysicists are not satisfied with the trough in the z=6.28 quasar. • A deeper understanding of the physics of reionization may be required • Some astrophysicists and cosmologists have turned to computer simulations

  21. Work Cited • http://nedwww.ipac.caltech.edu/level5/Sept01/Rauch/Rauch4.html • http://www.seds.org/~rme/cosmol.html • http://astron.berkeley.edu/~mwhite/darkmatter/bbn.html • http://astron.berkeley.edu/~john/lya.html • http://nedwww.ipac.caltech.edu/level5/March01/Barcana/Bar1.html • http://www.ticam.utexas.edu/CCV/projects/DiDi/cosmo/cosmo.html • SPECTRA OF THE MOST DISTANT QUASARS ELUCIDATE THE REIONIZATION OF THE COSMOS, By Schwarztschild, Bertram, Physics Today, 00319228, Oct2001, Vol. 54, Issue 10 (Database: MasterFILE select) • Cosmic Coincidences: Darkmatter, Mankind and anthropic cosmology, by John Bribbin and Martin Rees • http://www.scienceagogo.com/news/20010710012750data_trune_sys.shtml

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