PPT-Detecting Dark Energy with Atom Interferometry
Author : phoebe-click | Published Date : 2016-09-14
Clare Burrage University of Nottingham ClareBurragenottinghamacuk Outline Chameleon dark energy A review of atom interferometry Dark energy in the laboratory Solutions
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Detecting Dark Energy with Atom Interferometry: Transcript
Clare Burrage University of Nottingham ClareBurragenottinghamacuk Outline Chameleon dark energy A review of atom interferometry Dark energy in the laboratory Solutions to the Cosmological Constant Problem. Susan Cartwright. University of Sheffield. Neutrinos and the Universe. Discovering neutrinos. Detecting neutrinos. Neutrinos and the Sun. Neutrinos and Supernovae. Neutrinos and Dark Matter. Neutrinos and the Universe. Josh Frieman. Fermilab. and the University of . Chicago. Astronomy 41100. Lecture 2, Oct. 15, 2010. DES Collaboration Meeting. 2. Go to:. http://astro.fnal.gov/desfall2010/Home.html. Science Working group meetings on Tuesday.. This . powerpoint. will show you the basics of dark matter and dark energy . Their place in the universe . By Jordan . Ilori. . DARK MATTER. Dark matter is a type of matter hypothesized in astronomy and cosmology to account for a large part of the mass that appears to be missing from the universe. Dark matter cannot be seen directly with telescopes; evidently it neither emits nor absorbs light or other electromagnetic radiation at any significant level. Instead, the existence and properties of dark matter are inferred from its gravitational effects on visible matter, radiation, and the large-scale structure of the universe. According to the Planck mission team, and based on the standard model of cosmology, the total mass–energy of the known universe contains 4.9% ordinary matter, 26.8% dark matter and 68.3% dark energy. Thus, dark matter is estimated to constitute 84.5% of the total matter in the universe and 26.8% of the total content of the universe.. Jon Coleman, Royal Society Research Fellow . To detect and measure effects of Dark Energy density or any dark contents of the vacuum (DCV) . 2. Many thanks to the support of the:. Liverpool Particle Physics Group. limits on . dark . energy. Jun. 17. 2011. Geena Kim. P. Hamilton, D. Schlippe, and H. Mueller. University of California, Berkeley. Paul Hamilton. Müller group. University of California at Berkeley. . FOR DETECTING SURFACE DISPLACEMENT IN HILLY AREAS Noorlaila Hayati 1 , Muhammad Taufik 2 , Khomsin 3 Departmen t of Geomatics Engineering, The Faculty of Civil and Planning Sepuluh Nopember Institu Martin Kunz. University of . Geneva & AIMS South Africa. outline. what is the problem?. . dark energy theory. action based models. phenomenological approach. observations. simple principles. current constraints from Planck+. Observations. Josh . Frieman. DES Project Director. Fermilab. and the University of Chicago. Science with a Wide-. Field Infrared Telescope in Space. Pasadena, February. 2012. 2. 2011 Nobel Prize in Physics. Josh Frieman. Fermilab. and the University of . Chicago. Astronomy 41100. Lecture 2, Oct. 15, 2010. DES Collaboration Meeting. 2. Go to:. http://astro.fnal.gov/desfall2010/Home.html. Science Working group meetings on Tuesday.. Expansion of the Universe. Early 1990’s – Universal expansion expected to slow. . - Universe is full of matter, and gravity pulls matter together. 1998 – Hubble Space Telescope observations show otherwise. August 19, 2015. PROBING the MYSTERY: THEORY & EXPERIMENT in QUANTUM GRAVITY. . Galiano. Island. Tests of gravity and the quantum superposition principle using atom interferometry. Quantum superposition at the meter scale. Tim Kovachy. Department of Physics and Astronomy and Center for Fundamental Physics, Northwestern University. NPS Colloquium. February 1, 2019 . Conceptual overview of atom interferometry. Motivation for gravitational wave detection in the “mid-band” frequency range of ~ 0.1 Hz to 10 Hz. Tim Kovachy. Department of Physics and Astronomy and Center for Fundamental Physics (CFP), Northwestern University. CPAD 2021. Brief overview of atom interferometry. Enabling technology advances for large-area/long-baseline atom interferometry demonstrated with 10-meter baselines. Bohr’s Model . Niels. Bohr suggested that the problem about hydrogen spectrum can be solved if we can make some assumptions. . According to classical theory, the frequency of the electromagnetic waves emitted by a revolving electron is equal to the frequency of revolution. .
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