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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

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!

By jacob
(278 views)

UEET 603 Introduction to Energy Engineering Spring 2010

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.

By andrew
(271 views)

Summary of the Multi-Messenger Astronomy Workshop

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!

By johana
(326 views)

Science news

Science news

Science news Lots of it is about “gene therapy” Early (bad) problems: Results not reproducible And some deaths Recent successes “Curing” blindness of some kinds and to a degree “Arresting” a fatal syndrome Is there new life (one year more of funding) for the Tevatron?

By LeeJohn
(208 views)

ASTROPARTICLES IN THE LHC ERA

ASTROPARTICLES IN THE LHC ERA

NO - VE 2008, Venice, April 15-18, 2008. ASTROPARTICLES IN THE LHC ERA. Antonio Masiero Univ. of Padova and INFN, Padova. LHC and “LOW-ENERGY” NEW PHYSICS. LHC discovers NP : difficult, if not impossible, to “reconstruct” the fundamental theory lying behind those signals of NP;

By sherlock_clovis
(218 views)

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

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

neutrinos in cosmology. Strasbourg , 11 July 200 6 Julien Lesgourgues (LAPTH , Annecy ). acc élé ration. d écélé ration lente. d écélé ration rqpide. acc élé ration. inflation. radiation. mati è re. é nergie noire. The standard cosmological model. acc élé ration. acc ele ration.

By andrew
(266 views)

Dark Matter

Dark Matter

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

By Gabriel
(651 views)

PH599 Graduate Seminar presents: Discovery of Top Quark

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.

By matty
(301 views)

Layers of the sun

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.

By khoi
(1376 views)

Neutrino Novelties: Pointers to new physics?

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

By enoch
(183 views)

Announcements

Announcements

Announcements. Pick up “A,B,C,D” cards. Please bring them to class with you. Bring a calculator to lab. In many cases, you will need it. Course book “ A Tour of the Subatomic Zoo ” is available at Bookstore until April 15. So, please purchase it asap.

By meriel
(95 views)

Modern Physics

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 .

By loan
(332 views)

Fundamental Particles (The Standard Model)

Fundamental Particles (The Standard Model)

Fundamental Particles (The Standard Model). Nathan Brown June 2007. Part I. Fundamental Particle – The Meaning. It is understood that the universe is composed of particles. Democritus (born 450 BC, Greece) first introduced the particle nature of creation.

By joshua
(180 views)

Physics impact of Applied Antineutrino Detector Development

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

By olive
(132 views)

The structure and evolution of stars

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

By lana
(143 views)

Reflections on Symmetries and Neutrinos

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.

By balin
(131 views)

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 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.

By albert
(270 views)

Chapter 15: The Sun: A Nuclear Powerhouse

Chapter 15: The Sun: A Nuclear Powerhouse

Chapter 15: The Sun: A Nuclear Powerhouse. Happy Sun. Why Does the Sun Shine?. The Sun gives off energy (duh)! The energy must come from somewhere - there’s no free lunch. Conservation of energy is a fundamental tenet of physics. Where does the energy come from?

By lynnea
(139 views)

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?

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.

By brittania
(156 views)

Main Sequence Lifetimes

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

By kohana
(115 views)

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