PPT-Effective Action for Gravity and Dark Energy

Sang Pyo Kim Kunsan Natl Univ COSMO Co sPA Sept 30 2010 U Tokyo Outline Motivation Classical and Quantum Aspects of de Sitter Space Polyakovs Cosmic Laser Effective Action for Gravity. Gravity Pilates Tina Gravity Danielle MIND STUDIO MONDAY TUESDAY WEDNESDAY THURSDAY FRIDAY SATURDAY SUNDAY 8:00 Spartacus Boot Camp Rick 9:30 Barre Marla/Danielle Fusion (L1-2) Naomi Hatha 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.. University of Edinburgh. + . CFHTLenS. Collaboration + . WiggleZ. Collaboration. March 2012. Testing the Laws of Gravity with . CFHTLenS. and . WiggleZ. Modified Gravity or Dark Matter?. NASA. Dark Matter. Challenges. . in the Post-Planck . Era. Scott Dodelson. Bay Area Particle Theory Seminar . Oct. 4, 2013. What are the pressing open problems in physics in lieu of the Planck results?. Theoretical . Challenges. 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+. Dark Energy and Dark Matter. Prof. Lawrence Wiencke. Department of Physics Engineering. Colorado School of Mines. Nov 9 2011. The Dark . Side. 95% of the. Universe Is Dark!. Energy budget of 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.. 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. In the developing world, . more than 784 million people do not have access to . clean drinking water.. This causes over 5,000 deaths per day, and . billions. of dollars in . medical bills . and. loss in economic productivity.. A. nswer 9/7/16. A hiker’s velocity begins at 1.8 m/s uphill and changes to 1.5 m/s uphill. How do you know that the hiker has a negative acceleration?. 4 Types of Friction. The 4 types of friction are: . Convert the following to scientific notation. Distance from Sun. : 92,960,000 . miles ____. Estimated Age of universe – 14,000,000,000. Convert the following to standard form. Speed of light = 9.0 * 10. . SYFTET. Göteborgs universitet ska skapa en modern, lättanvänd och . effektiv webbmiljö med fokus på användarnas förväntningar.. 1. ETT UNIVERSITET – EN GEMENSAM WEBB. Innehåll som är intressant för de prioriterade målgrupperna samlas på ett ställe till exempel:. Hirosi. . Ooguri. EPS-HEP Conference, 15 July . 2019. Caltech and . Kavli. IPMU. 1. It is often said that string theory predicts the vast landscape . of . vacua. and that . any effective field theory can be realized .