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Berkeley | NUC 162
 
 

15 sample documents related to NUC 162

  • Berkeley NUC 162
    Interaction of Electromagnetic Radiation with Matter N E 162 Lecture 5 Chapter 8 of Text book Jasmina Vujic Electromagnetic Radiation Its Nature and Properties: Dual Nature Wave properties: m1/sc (m/s) = Particle Properties: m = 0, E = h, p = E
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/Lecture5-emr.ppt
     
  • Berkeley NUC 162
    Interaction of Heavy Charged Particles with Matter NE162 Lecture 7 Chapter 5 of Text book JASMINA VUJIC Interaction of heavy charged particles with matter Heavy charged particles all charged particles other than the electron or positron Include:
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/Lecture7-hchp.ppt
     
  • Berkeley NUC 162
    Interaction of Electrons with Matter NE162 Lecture 8 Chapter 6 of Text book JASMINA VUJIC Interaction electrons with matter Energy-Loss Mechanisms (a) Collisions with electrons Ionization of atoms Excitation of atoms (b) Radiative losses Bre
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/Lecture8-eltr.ppt
     
  • Berkeley NUC 162
     
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/Lecture9-10-ntr.pdf
     
  • Berkeley NUC 162
    [1] Monte Carlo Sampling Methods Jasmina L. Vujic Nuclear Engineering Department University of California, Berkeley Email: phone: fax: vujic@nuc.berkeley.edu (510) 643-8085 (510) 643-9685 UCBNE, J. Vujic [2] Monte Carlo Monte Carlo is a computat
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/MCIntro.pdf
     
  • Berkeley NUC 162
    DOSIMETRIC QUANTITIES AND UNITS IMPARTED ENERGY, ED = For a given volume of matter of mass m, the energy imparted in some time interval is the sum of the energies (excluding rest-mass energies) of all charged and uncharged ionizing particles enterin
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/NE162_Lecture11a-dose-def.pdf
     
  • Berkeley NUC 162
    CHARACTERIZATION OF RADIATION FIELDS AND SOURCES Radiation field - refers collectively to the particles and their trajectories in some region of space or through some boundary Radiation field is characterized by the particle distribution in space,
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/Lecture11-radfields.pdf
     
  • Berkeley NUC 162
     
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/NE162_Lecture11b-dose.pdf
     
  • Berkeley NUC 162
     
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/NE162_Lecture14a.pdf
     
  • Berkeley NUC 162
     
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/Tables-Buildup.pdf
     
  • Berkeley NUC 162
     
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/Tables-Coeff.pdf
     
  • Berkeley NUC 162
     
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/BNCT.pdf
     
  • Berkeley NUC 162
    he Effect of Cosmic Radiation on Humans Sylvain Costes, MH Barcellos-Hoff Life Science Division, Lawrence Berkeley National Laboratory Berkeley CA 94720 svcostes@lbl.gov Outline Introduction Why do we care about cosmic radiation? What are HZE?
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/NE162_Lecture16.ppt
     
  • Berkeley NUC 162
    NE162: Homework 9 Jonathan Dreyer April 29, 2008 Homework 9 Open homework and copy files from pdf to local directory C:\\NE162 Important Notes Updated dose.m file included in pdf Homework due May 2 at 5pm Editting the MCNP Input Open phantom.
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/2008-04-29%20Lecture.pdf
     
  • Berkeley NUC 162
    History of Radiation The birth of atomic models NE162 Lecture 1 Chapter 1 and 2 of text book Jasmina Vujic At the end of the 19th century, many scientists did not realize they were on the edge of a revolution in physics The most important fundame
    http://www.nuc.berkeley.edu/dept/Courses/NE-162/Lecture1-history.ppt
     
 
 
 
 
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