Today: Quantum mechanics
... electron with more energy Stopping potential goes to zero at some critical frequency For light below that frequency, no electrons are ejected. ...
... electron with more energy Stopping potential goes to zero at some critical frequency For light below that frequency, no electrons are ejected. ...
Conservation of Energy Worksheet Name ______________________ 1)
... The boulder begins to fall. What is its potential energy when it is 500-m above the ground? Where did the “lost” potential energy go? ...
... The boulder begins to fall. What is its potential energy when it is 500-m above the ground? Where did the “lost” potential energy go? ...
General Properties of Light c = 3.0 x 108 m/s .
... Raman scattering or the Raman effect is the inelastic scattering of a photon. Inelastic scattering is a kind of scattering that the energy is not conserved so the incoming particle has different energy than the scattered particle. When light is scattered from an atom or molecule, most photons are el ...
... Raman scattering or the Raman effect is the inelastic scattering of a photon. Inelastic scattering is a kind of scattering that the energy is not conserved so the incoming particle has different energy than the scattered particle. When light is scattered from an atom or molecule, most photons are el ...
Guass`s Law for magnetism
... • 4 X 10-7 m to 7X 10-7 m (400 to 700 nm) • Electrons – Radio – running electrons up and down an antenna – Electrons moving within atoms and molecules – X-rays - Electrons are rapidly decellerated by striking ...
... • 4 X 10-7 m to 7X 10-7 m (400 to 700 nm) • Electrons – Radio – running electrons up and down an antenna – Electrons moving within atoms and molecules – X-rays - Electrons are rapidly decellerated by striking ...
Class15
... • ENERGY IS QUANTIZED • Electrons can absorb energy and move to a higher level; they can emit light and move to a lower level • In hydrogen the emitted light will have energy E = (13.6 ev)(1/nf2 – 1/ ni2) • The wavelength is given by l = hc/E = 1240(nm eV)/E • Energy levels of nearby atoms are sligh ...
... • ENERGY IS QUANTIZED • Electrons can absorb energy and move to a higher level; they can emit light and move to a lower level • In hydrogen the emitted light will have energy E = (13.6 ev)(1/nf2 – 1/ ni2) • The wavelength is given by l = hc/E = 1240(nm eV)/E • Energy levels of nearby atoms are sligh ...
EM Lecture Slides
... studied the properties of Electricity and Magnetism. He took a mathematical approach. He published his first scientific paper when he was 15 years old. The four mathematical equations Maxwell produced are ranked with Sir Isaac Newton's laws of motion and Albert Einstein's theory of relativity as the ...
... studied the properties of Electricity and Magnetism. He took a mathematical approach. He published his first scientific paper when he was 15 years old. The four mathematical equations Maxwell produced are ranked with Sir Isaac Newton's laws of motion and Albert Einstein's theory of relativity as the ...
Dispersion of Light by Prisms In the Light and Color unit of The
... orange, yellow, green, blue and violet. The separation of visible light into its different colors is known as dispersion. It was mentioned in the Light and Color unit that each color is characteristic of a distinct wave frequency; and different frequencies of light waves will bend varying amounts up ...
... orange, yellow, green, blue and violet. The separation of visible light into its different colors is known as dispersion. It was mentioned in the Light and Color unit that each color is characteristic of a distinct wave frequency; and different frequencies of light waves will bend varying amounts up ...
924 Lecture, Energy
... The wavelength of maximum emission depends inversely on a body’s Kelvin temperature. max = 2897/T (microns) Emission from hotter bodies peaks at shorter wavelengths. What is max for the Sun? max = C/T = 2897/ 6000 = 0.48 microns = yellow visible light ...
... The wavelength of maximum emission depends inversely on a body’s Kelvin temperature. max = 2897/T (microns) Emission from hotter bodies peaks at shorter wavelengths. What is max for the Sun? max = C/T = 2897/ 6000 = 0.48 microns = yellow visible light ...