PPT-Physics of the Cosmos

Sections 374 375 Reminders Today Inclass Quiz 6 addressing Chapter 37 and questions from prior quiz and test LAB B2WNL Wave Nature of Light due Friday 4pm Weekly Reflection 13 will be sent out after class today due Tuesday evening after fall break. Middle Earth Summer Conference Office 9498242956 Please email the program coordinator at ganjuciedu for nonurgent nonemergency questions or confirmations P57352K57347H57347MH5734757347KM57347LMKM OSMOS 2014 has a class of 164 students from 20 Califo : . National Center for Atmospheric . Research. w. ith a whole lot of help from:. Jeff Anderson, . Nancy Collins, Kevin . Raeder, Bill Sacks. : . NCAR. Yongfei. Zhang. : . University of Texas . Austin. . Statistics. : . 1.8 . Ms. ½. . sq. .deg. . @. 160 . ksec. 1761 . sources. Dec. ’06-June ’07. Catalog. : . Elvis . et. al., . 2009, ApJS 184, 158. Martin Elvis, Francesca . Civano. , . Aldcroft. Sierra . Critical Zone Observatory. 3. rd. Annual COSMOS Workshop. Matthew Meadows. Sierra . Nevada Research . Institute. University . of California . Merced. Critical Zone Observatories. http://criticalzone.org. POWER . RADIO. GALAXIES AS BEACONS FOR CLUSTERS . AT . 1<z<2. Marco Chiaberge. INAF-IRA. Space Telescope Science Institute. A. . Capetti. INAF- OATO. G. Tremblay RIT. P. . Tozzi. INAF-OATS. Art & Drones . mix . the most futuristic technology scenarios with our aerial h. oop . d. rone performances, known as Cosmos Drones. See the video at:. https://youtu.be/5-9lk_y7vJs. Cosmos Drones . A Single Form, Mixing Diagram,. and Outliers . Heng Hao (SISSA). Martin Elvis (CFA). and COSMOS Team. INAF-OABO . Seminar. 2012-10-25 . 10%. 90%. Outline. Introduction: Definition . and Important Questions . SOF + SMV + RBV. SOF + SMV. Randomisation. 2 : 1 : 2 : 1*. Open-label. * . Randomisation. was stratified on genotype (1a or 1b) in both cohorts, . IL28B . in cohort 1 and treatment history (naïve or non-responder) in cohort . Andrew Liu. Program Manager. Azure OSSA + NoSQL. P4010. Raghav Mohan. Program Manager. Azure OSSA + NoSQL. Topics Covered. Brief overview of Azure Cosmos DB. Brief overview of Azure HDInsight. Data at Massive Scale. California State Summer School for Mathematics and Science. What is COSMOS?. “an intensive four-week summer residential program summer residential program for students who have demonstrated an aptitude for… STEM subjects”. The Night Sky. The Milky Way. Stars (individual, binary, variable). Clusters (globular and open). Nebulae (reflection, emission, dark, planetary). SNRs, Neutron Stars, & Black Holes. Galaxies. The Universe. pcos.gsfc.nasa.gov. Ann Hornschemeier . PCOS Chief Scientist. Expand our knowledge of dark energy. Precisely measure the cosmological parameters governing the evolution of the universe and test the inflation hypothesis of the Big Bang . pcos.gsfc.nasa.gov. Mark . Bautz. Massachusetts Institute of Technology. Chair of the Physics of the Cosmos Program Analysis Group. Increase our knowledge of dark energy. Precisely measure the cosmological parameters governing the evolution of the universe and test the inflation hypothesis of the Big Bang . Provides a physics-centered analysis of a broad range of astronomical systems that appeals to a large audience of advanced undergraduate students in physics and engineeringThis book gives a survey of astrophysics at the advanced undergraduate level. It originates from a two-semester course sequence at Rutgers University that is meant to appeal not only to astrophysics students but also more broadly to physics and engineering students. The organization is driven more by physics than by astronomy in other words, topics are first developed in physics and then applied to astronomical systems that can be investigated, rather than the other way around.The first half of the book focuses on gravity. Gravity is the dominant force in many astronomical systems, so a tremendous amount can be learned by studying gravity, motion and mass. The theme in this part of the book, as well as throughout astrophysics, is using motion to investigate mass. The goal of Chapters 2-11 is to develop a progressively richer understanding of gravity as it applies to objects ranging from planets and moons to galaxies and the universe as a whole. The second half uses other aspects of physics to address one of the big questions. While Why are we here? lies beyond the realm of physics, a closely related question is within our reach: How did we get here? The goal of Chapters 12-20 is to understand the physics behind the remarkable story of how the Universe, Earth and life were formed. This book assumes familiarity with vector calculus and introductory physics (mechanics, electromagnetism, gas physics and atomic physics) however, all of the physics topics are reviewed as they come up (and vital aspects of vector calculus are reviewed in the Appendix).