'Large cross section' presentation slideshows

INDUCTION MOTORS 3

INDUCTION MOTORS 3. INDUCTION MOTOR MAXIMUM TORQUE. maximum power transfer occurs when: R 2 /s=?R TH ^2 + (X TH +X 2 )^2 (1) solving (1) for slip ? s max = R 2 / ?R TH ^2 + (X TH +X 2 )^2 (2)

1.56k views • 83 slides

The Physics Case for CLIC

The Physics Case for CLIC. Outline of the CLIC project Why an e + e - collider with E CM = 3 TeV? A significant step beyond the LHC/ILC for precision measurements at high energies Complete study of the Higgs boson(s)? Supersymmetric spectra? Deeper probes of extra dimensions?

860 views • 73 slides

Status of meson photoproduction experiments with CLAS

779 views • 67 slides

Lecture 6 Jack Tanabe Old Dominion University Hampton, VA January 2011

563 views • 50 slides

Viscous hydrodynamic model for Relativistic Heavy Ion Collisions A. K. Chaudhuri

Viscous hydrodynamic model for Relativistic Heavy Ion Collisions A. K. Chaudhuri Variable Energy Cyclotron Centre, Kolkata . Introduction. Why (viscous) hydrodynamics? Hydrodynamical modeling of nuclear collisions. smooth hydrodynamics. initial condition, freeze-out,

571 views • 44 slides

Statistics and Data Analysis

430 views • 33 slides

QCD at CDF

410 views • 27 slides

Fueling Requirements for Steady State Spherical Torus Operation

Supported by. Fueling Requirements for Steady State Spherical Torus Operation. Roger Raman, Thomas R. Jarboe, + Henry W. Kugel University of Washington, Seattle + Princeton Plasma Physics Laboratory Joint Meeting of the 3rd IAEA technical Meeting on Spherical Torus

391 views • 23 slides

Coupling of (deformed) core and weakly bound neutron

344 views • 22 slides

Significant effects of second KK particles on LKP dark matter physics

Significant effects of second KK particles on LKP dark matter physics. Mitsuru Kakizaki (ICRR, University of Tokyo). March. 23, 2005 @ Univ. of Oxford. Collaborated with Shigeki Matsumoto (ICRR) Yoshio Sato (Saitama Univ.) Masato Senami (ICRR) hep-ph/0502059.

338 views • 21 slides

Relic abundance of dark matter in the Minimal Universal Extra Dimension model

in collaboration with Shigeki Matsumoto (KEK) Mitsuru Kakizaki (Bonn Univ.). Relic abundance of dark matter in the Minimal Universal Extra Dimension model. Masato Senami (ICRR, University of Tokyo) senami@icrr.u-tokyo.ac.jp. Phys. Rev. D 71, 123522 (2005)

369 views • 21 slides

M. Kimura(Hokkaido)

Systematic study of the many-particle and many-hole states in and around the Island of Inversion - #N=Odd system -. M. Kimura(Hokkaido). Introduction : Island of Inversion. Island of Inversion : N ? 20 Ne, Na, Mg isotopes Topics: large deformation, mpmh config ., shell gap quench

321 views • 20 slides

Project Attrition

Project Attrition. Presenter Name Presenter Title Presenter Employer. Project Attrition. Made possible by generous support from the meetings, conventions and exhibitions industry. Lead contributors are the foundations of: Meeting Professionals International (MPI)

536 views • 19 slides

PAID POLITICAL ADVERTISING A NARRATIVE PERSPECTIVE

PAID POLITICAL ADVERTISING A NARRATIVE PERSPECTIVE. Attributes shared by political spots summarized in six propositions. Proposition 1: The central purpose of political spots is to influence voter's perceptions of candidates.

272 views • 15 slides

Nucleon knockout reactions with heavy nuclei

Nucleon knockout reactions with heavy nuclei. Edward Simpson University of Surrey Brighton PRESPEC Meeting 12 th January 2011. Absolute cross sections. Momentum distributions. Nucleon knockout reactions. Cross section proportional to spectroscopic strength

287 views • 13 slides

Genesis Offices including The Genesis CDA Training and Resource Centre for the local community

1.18k views • 11 slides

Explorer Post 1010 TARC Team 8296

Explorer Post 1010 TARC Team 8296. Chris Fann Ronnie Foreman Phil Manougian Amanda Steckel. Design Process. We made use of the rocket design software, RockSim to digitally build and test our rocket before official production.

198 views • 8 slides

What Is Pop Culture?

305 views • 7 slides

ttH

ttH. Akimasa Ishikawa Saga University. ttH. m H =120 ~ 200 GeV ?s thre = m t *2+ m H = 470 ~ 550 GeV s (? s thre + a ) = O(0.1) fb ? O(100) events with 1000/fb ~1fb with m H =120GeV at 550GeV Decay ttH ? bWbW (WW or ZZ) ? 10 fermions All jet mode Lepton mode Tau mode

213 views • 4 slides