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    About 297 results
    • https://phys.libretexts.org/Bookshelves/Thermodynamics_and_Statistical_Mechanics/Supplemental_Modules_(Thermodynamics_and_Statistical_Mechanics)/Thermodynamics/1.13%3A_Heat_Transport
      Contributors and Attributions Michael Fowler (Beams Professor, Department of Physics, University of Virginia)
    • https://phys.libretexts.org/Bookshelves/Astronomy__Cosmology/Supplemental_Modules_(Astronomy_and_Cosmology)/Astronomy/Gravity
    • https://phys.libretexts.org/Bookshelves/Quantum_Mechanics/Quantum_Mechanics_(Fowler)/zz%3A_Back_Matter
    • https://phys.libretexts.org/Bookshelves/Quantum_Mechanics/Quantum_Mechanics_(Fowler)/00%3A_Front_Matter/02%3A_InfoPage
      The LibreTexts libraries are Powered by MindTouch ® and are supported by the Department of Education Open Textbook Pilot Project, the UC Davis Office of the Provost, the UC Davis Library, the Californ...The LibreTexts libraries are Powered by MindTouch ® and are supported by the Department of Education Open Textbook Pilot Project, the UC Davis Office of the Provost, the UC Davis Library, the California State University Affordable Learning Solutions Program, and Merlot.
    • https://phys.libretexts.org/Bookshelves/Quantum_Mechanics/Quantum_Mechanics_(Fowler)/04%3A_Angular_Momentum_Spin_and_the_Hydrogen_Atom/4.02%3A_Orbital_Eigenfunctions-_2-D_Case
      \[ -\dfrac{\hbar^2}{2M}(\dfrac{\partial^2}{\partial r^2}+\dfrac{1}{r}\dfrac{\partial}{\partial r}+\dfrac{1}{r^2}\dfrac{\partial^2}{\partial \phi^2})R_{E,m}(r)\Phi_m(\phi)+V(r)R_{E,m}(r)\Phi_m(\phi)=ER...22M(2r2+1rr+1r22ϕ2)RE,m(r)Φm(ϕ)+V(r)RE,m(r)Φm(ϕ)=ERE,m(r)Φm(ϕ),
    • https://phys.libretexts.org/Bookshelves/Thermodynamics_and_Statistical_Mechanics/Supplemental_Modules_(Thermodynamics_and_Statistical_Mechanics)/Thermodynamics/1.08%3A_The_Laws_of_Thermodynamics_and_Limits_on_Engine_Efficiency
      Contributors and Attributions Michael Fowler (Beams Professor, Department of Physics, University of Virginia)
    • https://phys.libretexts.org/Bookshelves/Quantum_Mechanics/Quantum_Mechanics_(Fowler)/03%3A_Mostly_1-D_Quantum_Mechanics
      Thumbnail: A particle in a 1D infinite potential well of dimension L.
    • https://phys.libretexts.org/Bookshelves/Classical_Mechanics/Graduate_Classical_Mechanics_(Fowler)/15%3A_Keplerian_Orbits/15.03%3A_Keplers_Statement_of_his_Three_Laws
      As a planet moves in its orbit, the line from the center of the Sun to the center of the planet sweeps out equal areas in equal times, so if the area SAB(with curved side AB) equals the area ...As a planet moves in its orbit, the line from the center of the Sun to the center of the planet sweeps out equal areas in equal times, so if the area SAB(with curved side AB) equals the area SCD, the planet takes the same time to move from A to B as it does from CtoD.
    • https://phys.libretexts.org/Bookshelves/Classical_Mechanics/Graduate_Classical_Mechanics_(Fowler)
      Thumbnail: Proper Euler angles geometrical definition. The xyz (fixed) system is shown in blue, the XYZ (rotated) system is shown in red. The line of nodes (N) is shown in green. (CC BY 3.0; Lionel Br...Thumbnail: Proper Euler angles geometrical definition. The xyz (fixed) system is shown in blue, the XYZ (rotated) system is shown in red. The line of nodes (N) is shown in green. (CC BY 3.0; Lionel Brits).​​​​​
    • https://phys.libretexts.org/Bookshelves/Classical_Mechanics/Graduate_Classical_Mechanics_(Fowler)/04%3A_Hamilton's_Principle_and_Noether's_Theorem
      She was described by Pavel Alexandrov, Albert Einstein, Jean Dieudonné, Hermann Weyl, and Norbert Wiener as the most important woman in the history of mathematics. As one of the leading mathematicians...She was described by Pavel Alexandrov, Albert Einstein, Jean Dieudonné, Hermann Weyl, and Norbert Wiener as the most important woman in the history of mathematics. As one of the leading mathematicians of her time, she developed the theories of rings, fields, and algebras. In physics, Noether's theorem explains the connection between symmetry and conservation laws.
    • https://phys.libretexts.org/Bookshelves/Classical_Mechanics/Graduate_Classical_Mechanics_(Fowler)/22%3A_Resonant_Nonlinear_Oscillations/22.06%3A_Frequency_Multiples
      We’ve only considered a quartic addition to the potential, 14βx4, a force βx3, we can show that gives a resonance near γ=13ω0, and ...We’ve only considered a quartic addition to the potential, 14βx4, a force βx3, we can show that gives a resonance near γ=13ω0, and presumably this is the small bump near the beginning of the curves above for large driving strength.

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