'Neutrinos' diaporamas de présentation

Main Sequence Lifetimes

Main Sequence Lifetimes. Time on Main Sequence How much fuel it has (Core H) How fast it consumes the fuel (Luminosity). Main Sequence Lifetimes. Main Sequence Lifetimes. Our Sun M = 1 M ( ?) and L = 1 L ( ?) t MS -lifetime = 10 10 years = 10 billion years

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Big Bang, Black Holes, No Math ASTR/PHYS 109 Dr. David Toback Lecture 23 & 24

Big Bang, Black Holes, No Math ASTR/PHYS 109 Dr. David Toback Lecture 23 & 24 Papers Paper 1 is done Paper 2 grades are on eLearning All grades fixed, revision paper grades posted Paper 3: We have fixed papers for calibration problems Still mis-graded? Let us know!

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ASTROPARTICLES IN THE LHC ERA

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Summary of the Multi-Messenger Astronomy Workshop

Summary of the Multi-Messenger Astronomy Workshop Garmt de Vries Les Houches, 2002 Multi-Messenger Astronomy Workshop Organisers: D. Smith & A. Barrau 2 sessions planned 2 sessions added Goal of the workshop: To dive into the wonderful world of astrophysical catalogues!

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UEET 603 Introduction to Energy Engineering Spring 2010

UEET 603 Introduction to Energy Engineering Spring 2010 Nuclear Power Nuclear Energy Nuclear energy is a way of creating heat through the fission process of atoms. Nuclear energy originates from the fission of atomic nucleus in a chain reaction.

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Fundamental Particles (The Standard Model)

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Reflections on Symmetries and Neutrinos

Reflections on Symmetries and Neutrinos. Adam Para. Revolutionary Developments in XX Century Physics. Special Relativity General Relativity Quantum Mechanics Quantum Field Theory Standard Model of Elementary Particles and their Interactions Role of symmetry in physics.

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Chapter 15: The Sun: A Nuclear Powerhouse

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Strasbourg , 11 July 200 6 Julien Lesgourgues (LAPTH , Annecy )

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What should we do with the problem arising from the poorly made photocopies?

What should we do with the problem arising from the poorly made photocopies?. A. Decrease the percentage earned for the midterm. B. Have a new midterm exam. C. Have a new short exam in addition to the final. D. Make the judgment on the basis of first 11 questions.

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Neutrino Novelties: Pointers to new physics?

Neutrino Novelties: Pointers to new physics?. DAE Golden Jubilee Colloquium Institute of Mathematical Sciences, Chennai May 19, 2004 Amitava Raychaudhuri University of Calcutta. Neutrino Novelties. Experimental results: solar and atmospheric neutrinos

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Modern Physics

Modern Physics. Introduction. To examine the fundamental nuclear model To examine nuclear classification To examine nuclear fission and fusion. Detection Devices. Geiger counter Scintillation counter Cloud chamber Bubble chamber Superheated liquid. Fundamental Particles .

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PH599 Graduate Seminar presents: Discovery of Top Quark

PH599 Graduate Seminar presents: Discovery of Top Quark. Karen Chen Stony Brook University November 1, 2010. Abstract.

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Announcements

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The structure and evolution of stars

The structure and evolution of stars. Lecture13: Supernovae - deaths of massive stars. Complete notes available online: http://star.pst.qub.ac.uk/~sjs/teaching.html. Learning Outcomes. In these final two lectures the student will learn about the following issues: What is a supernova

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Dark Matter

Dark Matter. Mike Brotherton Professor of Astronomy, University of Wyoming Author of Star Dragon and Spider Star. The Father of Dark Matter.

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Science news

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Outline of a Program in Investigating Nucleon and Nuclear Structure at all Q 2 - Starting with P 04-001 ( PART 1 of J

Outline of a Program in Investigating Nucleon and Nuclear Structure at all Q 2 - Starting with P 04-001 ( PART 1 of JUPITER program ) (a) Study Nucleon Structure and Nuclear Effects (b) Provide basic measurements needed for the next generation neutrino oscillation experiments.

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Physics impact of Applied Antineutrino Detector Development

Physics impact of Applied Antineutrino Detector Development. Giorgio Gratta Physics Department, Stanford. Bragging rights Synergy/collaboration Compact detectors No/light shielding is good Very large detectors Reliable/stable detectors. Neutrinos have a rich history of synergies

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Layers of the sun

Layers of the sun. Core Rad zone Convection zone Photosphere Chromosphere Corona Solar wind. Proton-Proton chain. Main source of fusion in core Two protons come together One proton changes to neutron, forming deuterium Note that a positron and neutrino are ejected.

2.26k views • 9 slides