19. Quantum Physics

Quantum Physics Photoelectric effect is the ejection of an electron from a metal surface when the surface is irradiated with electromagnetic radiation of a high enough frequency. Work function energy is the minimum energy required to eject an electron from a metal surface in the photoelectric effect. Stopping potential is the minimum value of the retarding potential difference required to prevent any photoelectron (not even those with maximum kinetic energy) from reaching the collector. smax eV =KE eV = vm smaxe 2 2 1 A photon is a quantum of electromagnetic energy. E = hf λ hc = E Intensity of electromagnetic radiation Power of the incident electromagnetic beamIntensity = Area of surface exposed to radiation Total energy incident = Area of surface exposed to radiation x time Nf= Intensity tA NE Nhf At At     Einstein’s Photoelectric Equation maxKE + φ = hf Threshold frequency fo is the minimum frequency of electromagnetic radiation incident on a metal surface required for photoelectric effect to take place, that is, to eject electrons from that surface. = φ 0hf maxKE + hf = hf 0

Wave-Particle Duality While the interference and diffraction phenomena of electromagnetic radiation prove the wave nature of electromagnetic radiation, the photoelectric effect provides evidence for the particulate nature of electromagnetic radiation. This shows the wave -particle duality of electromagnetic radiation. This led de Broglie to suggest that matter might also exhibit this duality and have wave properties. de Broglie Wavelength p h =  Energy levels As shown below is an example of an energy level diagram showing 2 electron energy levels. As a result of absorbing the exact amount of energy (E), an electron can transit from a lower energy level (E1) to a higher energy level (E2). At E2, the electron is said to be in an excited state. The electron is in an unstable state, and it will return rapidly and spontaneously to a lower energy level. As shown below i s the de-excitation of the atom in which the electron falls back from E 2 to E1, and the energy difference E is emitted as a photon (a burst of electromagnetic radiation) of a particular frequency f.

Line Spectra Emission Line Spectrum In an emission line spectrum, bright coloured lines are seen against a dark background. Absorption Line Spectrum In an absorption line spectrum, dark lines are seen against a continuous coloured background.

X-rays A common way for producing X-rays is by firing a beam of high-speed electrons at a metal target. The processes involved in X-ray emission includes Bremsstrahlung and transitions of target atom’s electrons. An X-ray spectrum is observed from the experiment and is represented as a graph of relative intensity of X-rays against X-ray wavelength. limits) hlung(Bremsstra eV hc=λ eV = λ hc eVhf electron incident of KE of lossTota