Loading [MathJax]/jax/output/HTML-CSS/jax.js
Skip to main content
Library homepage
 

Text Color

Text Size

 

Margin Size

 

Font Type

Enable Dyslexic Font
Physics LibreTexts

Search

  • Filter Results
  • Location
  • Classification
    • Article type
    • Author
    • Embed Hypothes.is?
    • Embebbed CalcPlot3D?
    • Cover Page
    • License
    • Show TOC
    • Transcluded
    • OER program or Publisher
    • Student Analytics
    • Autonumber Section Headings
    • License Version
    • Print CSS
      • Screen CSS
      • PrintOptions
    • Include attachments
    Searching in
    About 4 results
    • https://phys.libretexts.org/Learning_Objects/A_Physics_Formulary/Physics/14%3A_Nuclear_Physics
      Nuclear physics, radiative decay processes, nuclear binding and structure
    • https://phys.libretexts.org/Bookshelves/Nuclear_and_Particle_Physics/Introduction_to_Applied_Nuclear_Physics_(Cappellaro)/01%3A_Introduction_to_Nuclear_Physics/1.02%3A_Binding_energy_and_Semi-empirical_mass_formula
      The total binding energy is instead the difference between the interaction of a nucleon to its neighbor and the kinetic energy of the nucleon itself. This correction (and the following one) can only b...The total binding energy is instead the difference between the interaction of a nucleon to its neighbor and the kinetic energy of the nucleon itself. This correction (and the following one) can only be explained by a more complex model of the nucleus, the shell model, together with the quantum-mechanical exclusion principle, that we will study later in the class.
    • https://phys.libretexts.org/Courses/Georgia_State_University/GSU-TM-Introductory_Physics_II_(1112)/zz%3A_Back_Matter/10%3A_13.1%3A_Appendix_J-_Physics_Formulas_(Wevers)/1.14%3A_Nuclear_Physics
      Nuclear physics, radiative decay processes, nuclear binding and structure
    • https://phys.libretexts.org/Bookshelves/University_Physics/Radically_Modern_Introductory_Physics_Text_II_(Raymond)/13%3A_Newtons_Law_of_Gravitation/13.07%3A_Use_of_Conservation_Laws
      where m is the mass of the bullet, M is the mass of the moon, R is the radius of the moon, and v initial is the minimum initial velocity required for the bullet to escape. At apheli...where m is the mass of the bullet, M is the mass of the moon, R is the radius of the moon, and v initial is the minimum initial velocity required for the bullet to escape. At aphelion and perihelion, the radial part of the velocity of the asteroid is zero and the speed equals the tangential component of the velocity, v = v t . Thus, at aphelion and perihelion we can eliminate v in favor of the angular momentum:

    Support Center

    How can we help?