'Direct detection' presentation slideshows

The Search for Gravitational Waves Barry Barish Caltech University of Iowa 16-Sept-02

The Search for Gravitational Waves Barry Barish Caltech University of Iowa 16-Sept-02. Newton Universal Gravitation. Three laws of motion and law of gravitation (centripetal force) disparate phenomena eccentric orbits of comets cause of tides and their variations

936 views • 63 slides

James L. Pinfold University of Alberta

AstroCollider Physics. ASTROPARTICLE PHYSICS AND THE LHC. James L. Pinfold University of Alberta. Menu. The LHC and its multi-purpose detectors, for high p t physics (and forward physics?) Forward physics at the LHC and Cosmic Ray physics The cosmic ray energy spectrum

831 views • 50 slides

634 views • 38 slides

NexGen NPOESS Wind Observing Sounder: NASA/GSFC IDL Study and Findings

NexGen. NexGen NPOESS Wind Observing Sounder: NASA/GSFC IDL Study and Findings. Prepared for Mr. Dan Stockton, Program Executive Officer Program Executive Office for Environmental Satellites Presented by Dr. Wayman Baker NOAA/NASA/DoD Joint Center for Satellite Data Assimilation and

560 views • 38 slides

Laboratory Diagnosis of Viral Infection

1.78k views • 37 slides

Lectures 9-10

Lectures 9-10. Particle interactions with matter. 9.0 Overview. 9.3 Photons in matter Overview Photoelectric effect Raleigh scattering Compton scattering Pair production Comparison of cross-sections Z & A dependence of cross-sections

611 views • 34 slides

The Dark Side of the Universe

The Dark Side of the Universe . Lecture 26. Homework. Read Ch. 24: Life in the Universe HW: MasteringAstronomy Chapter 24. Final Exam. Time: Thursday, Dec 13 at 11:30am in VLSB2050 . Topics: - 25 % material covered before midterm 1 .

522 views • 33 slides

Indirect Searches for Dark Matter with CTA

Aquarius, Springel et al. arXiv:0809.0898. Indirect Searches for Dark Matter with CTA. Brian Humensky, for the CTA Consortium Columbia University Cosmic Visions, University of Maryland March 24, 2017. Dark Matter Searches. Cherenkov Telescope Array Concept & Timeline

444 views • 32 slides

Microbiology ST-2 Physiology and metabolism

438 views • 30 slides

Pulse and Pulse Processing

Pulse and Pulse Processing. Supriya Das Centre for Astroparticle Physics and Space Science Bose Institute supriya@bosemain.boseinst.ac.in 4 th. Winter School on Astro-Particle Physics (WAPP 2009) Mayapuri, Darjeeling. Measure what is measurable, and make measurable what is not so.

1.94k views • 28 slides

A Geosynchronous LIDAR Observatory For Atmospheric Winds And Moisture Measurements

A Geosynchronous LIDAR Observatory For Atmospheric Winds And Moisture Measurements. G. D. Emmitt Simpson Weather Associates G. D. Spiers CalTech/JPL. Revolutionize our ability to monitor and predict severe atmospheric events on a routine basis tropical cyclone tracks and intensity

386 views • 24 slides

intro to neutralino dark matter

364 views • 23 slides

Neutrinos y materia oscura

317 views • 21 slides

B. pseudomallei : Role of MALDI-TOF

534 views • 20 slides

Gravitational Waves at the AEI

Gravitational Waves at the AEI. Bernard Schutz. Bernard.Schutz@aei.mpg.de. Themes. General relativity impacts astrophysics broadly today: black holes, neutron stars, gravitational lensing, cosmology, gravitational waves.

415 views • 20 slides

Search for Dark Matter

Search for Dark Matter. physics 805 fall 2008. WIMP search strategies. Direct detection

297 views • 19 slides

Results from Borexino

Results from Borexino. NOW 2012 September 9-16, 2012. Davide Franco CNRS-APC. Detector layout and radiopurity. Stainless Steel Sphere: 2212 PMTs 1350 m 3. Scintillator: 270 t PC+PPO in a 150 m m thick nylon vessel. Water Tank: g and n shield m water ? detector

286 views • 19 slides

Direct and Indirect Dark Matter Detection in Models with a Well-Tempered Neutralino

Direct and Indirect Dark Matter Detection in Models with a Well-Tempered Neutralino. Eun-Kyung Park Florida State University in collaboration with H. Baer (FSU), A. Mustafayev (U. of Kansas) and X. Tata (U. of Hawaii) : JCAP 0701 (2007) 017. OUTLINE. Overview of the mSUGRA model

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Welcome to the First CLASH Science Team Meeting

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E/O and O/E devices, the collaboration with the industry:

Analogue optical links experiences in the framework of the SKA/BEST activities. Federico Perini. INAF-IRA (I). Motivation: Necessity to bring the signal from the BEST Front End, on the antenna focal lines, to the central processing room.

112 views • 1 slides