PPT-1 Cosmology with Supernovae:

Lecture 2 Josh Frieman I Jayme Tiomno School of Cosmology Rio de Janeiro Brazil July 2010 Hoje V Recent SN Surveys and Current Constraints on Dark Energy VI Fitting SN Ia Light Curves amp Cosmology . Supernovae . J081659.74+511233.7 . and . J07285387+3349106. . with . the BSU . Observatory. Benjamin . Lombard and Sarah Peck . (Mentor: Professor Jamie Kern). Bridgewater State University. Abstract. Fall . 2012. Cosmology 2012. Cosmology I & II. Cosmology I: . 4. .9. .-. 21.10. .. Cosmology II: . 29. .10. .. -. 16.12. .. http://theory.physics.helsinki.fi. /. ~. cosmology. Lectures in A315, Mon & Tue 14.15-16.00. Edwin Hubble. S.B. ’10, Ph.D. ‘17. Hubble . constant. Hubble law. Hubble diagram. Hubble age. Hubble classification. Hubble radius. Hubble sequence. Hubble . flow. Hubble volume. …. .. Pretty much invented observational cosmology & . Array for Sub-. F. ermi . E. nergy . H. eavy Ion . R. eaction . D. ynamics. Summer REU Program 2012. Brittany Abromeit. August 3, 2012. 1. Outline:. Supernovae and the resulting neutron stars. Nuclear Equation of State. Talk by: John McCann. Paper by: D. . Poznanski. , Z. Kostrzewa-Rutkowska, L. Wyrzykowski & N. . Blagorodnova. OGLE-IV. OGLE – Optical Gravitational Lensing Experiment, Phase four. Las . Lecture 2. Josh . Frieman. I Jayme . Tiomno. School of Cosmology, Rio de Janeiro, Brazil. July 2010. Hoje. V. Recent SN Surveys and Current Constraints on Dark Energy. VI. Fitting SN . Ia. Light Curves & Cosmology . Astronomy 123. Cosmology. Cosmology is the empirical study of the organization, structure and evolution of the Universe. At any given time we always think our Cosmology is correct: . Ancient: Earth is at center of Universe. Developed by . the SOFIA Team. 0. Topic: . Supernovae.. Concepts: . Supernovae, planet formation, infrared observations. Missionb. : . SOFIA. Coordinated by: . the NASA Astrophysics Forum. An Instructor’s Guide for using the slide sets is available at the ASP website . Mysterious explosions in the Universe. Poonam Chandra. Royal Military College of Canada. Universe is 14 billion years old.. Our sun is 5 billion years.. Supernovae and Gamma ray bursts. Explosions lasting fraction of a second to few seconds.. light curves and spectral evolution. Bruno . Leibundgut. ESO. The core-collapse SN poster child. SN 1987A. the best observed supernova ever. Suntzeff. (2003). (also . Fransson. et al. 2007). What do we want to learn about supernovae?. Most stars either have M < 1.4 . M. ʘ. , . or can lose enough mass during post-main sequence evolution to get there, and end as white dwarf. However if core is more massive, nothing can stop gravitational collapse. University of Sheffield. What is a supernova?. Stellar explosions. Types of supernova. The importance of. supernovae. Supernova remnants. Stellar explosions. Most stars are a balancing act between gravity and pressure. Lecture 1. Josh . Frieman. I Jayme . Tiomno. School of Cosmology, Rio de Janeiro, Brazil. July 2010. Hoje. I. Cosmology Review. II. Observables: Age, Distances. III. Type . Ia. Supernovae as . Standardizable. Florida State University. YSP. Topics. Big . Bang Cosmology. The Accelerating Universe. Summary. Big . bang . cosmology. 3. In . the distant past the visible Universe was much smaller than it is today and therefore much, much hotter..