PPT-Cosmic Acceleration Then and

Now Josh Frieman Fermilab and the University of Chicago Progress on Old and New Themes in Cosmology Avignon April 18 2014 Last Supper in earlier version of program Cosmologists discuss BICEP2 results at PONT banquet. vs. GZK . …. … heavy composition . vs. anisotropies. Martin Lemoine. Institut d’Astrophysique de Paris. CNRS, Université Pierre & Marie Curie. M. . Lemoine & E. Waxman, . arXiv:0907.1354. AronsFest. 1. Anisotropic . Plasma. . Astrophysics. Roger . Blandford. Paul Simeon. Yajie. Yuan. KIPAC. Stanford. 27 i 2012. AronsFest. 2. Describing Cosmic Plasma. Fluid description. P. , . . , . & Large scale structure. Tarun Souradeep. I.U.C.A.A. .. Cosmology . IUCAA . VSP program. (. May 18-22, . 2012). Lec. . . 4:. Current frontiers. Mildly Perturbed universe at z=1100. Present universe at z=0. at. . Hartnell. . College. : A Case Study in Successful Undergraduate Research at a Two-Year College. Leo . Osornio. Hartnell. College. Presented at the 2012 AAPT Summer Meeting, Philadelphia. July 30, 2012. and Other Applications: Hydrology +. Neutron Monitor Community Workshop—Honolulu, Hawaii . October . 24-25, 2015. Physicist. National Urban Security Technology Laboratory . Science and Technology Directorate. Indonesia has a long history of the sculptural arts. Megalithic images are found in archeological sites in Sumatra, Java to Sulawesi. The 8-10. th. century sculptures and reliefs found in Java and Bali of Hindu-Buddhist origins reveal foreign influences. Indigenous tribes developed their own distinct tribal styles created as ancestor, deity and animal memorial sculptures. . Dave Ector. COSMIC PM for OSD. 4 November 10. COSMIC 2. 2. Requirements. GNSSRO Level . 1 . Requirements Documents (L1RD) . status. L1RD Completed and signed 5 May 2010. L1RD assessment underway. Initial budget/partnerships for COSMIC-2 do not fully support all L1RD requirements. Heino Falcke . Radboud University, Nijmegen. ASTRON, . Dwingeloo. What we (don’t) know about UHECRs . We know:. their energies (up to 10. 20. eV).. their overall energy spectrum. We don’t know:. Describe the speedometer on a car that is entering a highway, drives for 25 miles and then exits the highway.. Consider the two situations below. When a shuttle bus approaches a stop, the driver begins to apply the brakes to slow down 5.0 s before actually reaching the stop. The speed changes from 9.0 m/s to 0 m/s over time.. Acceleration is a change in velocity. Speed or direction. Centripetal Acceleration. Acceleration can mean a change in direction, not just speed. Centripetal acceleration. Acceleration that occurs in a circular motion. (LEP and LHC experiments). Arturo . Fernández. , Mario Rodriguez. Facultad. de . Ciencias. . Físico. . Matemáticas. Benemérita. Universidad Autonoma de Puebla. Manaus, Brazil Aug. 3. rd. 2015. Plasma. . Astrophysics. Roger . Blandford. Paul Simeon. Yajie. Yuan. KIPAC. Stanford. 27 i 2012. AronsFest. 2. Describing Cosmic Plasma. Fluid description. P. , . . , . v. , B…. Magneto Fluid Dynamics . Eun-Suk. . Seo. Inst. for Phys. Sci. & Tech. and . Department of Physics. University of Maryland. AAS HEAD meeting, Chicago, IL, 19 August 2014. w. ith edits & voice from . Angela V. Olinto. Vikram . Dwarkadas. . (U Chicago). Matthieu. Renaud, . Alexandre. . Marcowith. . (LUPM, U Montpellier). Vincent . Tatischeff. . (. Univ. Paris-. Sud. ). August 11 2017. TevPA 2017 : VVD. 1. We acknowledge support from the FACCTS program at .