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Electromagnetic Radiation: Wavelength, Frequency, and Energy, Study notes of Chemistry

Information on the concepts of electromagnetic radiation, including wavelength, frequency, amplitude, and energy. It includes examples of calculating the frequency and energy of different types of electromagnetic radiation, such as x-rays and radio waves. It also discusses the photoelectric effect and the relationship between energy and frequency.

Typology: Study notes

Pre 2010

Uploaded on 03/18/2009

koofers-user-hm1
koofers-user-hm1 🇺🇸

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Download Electromagnetic Radiation: Wavelength, Frequency, and Energy and more Study notes Chemistry in PDF only on Docsity! Electromagnetic Radiation ¥ WAVELENGTH (λ) - The distance between identical points on successive waves. ¥ FREQUENCY (ν) - The number of waves that pass through a particular point per second. ¥ AMPLITUDE - The vertical distance from the midline to a peak, or trough in the wave. λ = c ν Fig 7.1 (P 260) Fig 7.2 (P 260) The Spectrum of Electromagnetic Radiation ¥ The Wavelength of Visible light is between 400 and 700 nanometers ¥ Radio, TV , Microwave and Infrared radiation have longer wavelengths (shorter frequencies), and lower energies than visible light. ¥ Gamma rays and X-rays have shorter wavelengths (larger frequencies), and higher energies than visible light! Calculation of Frequency from Wavelength Problem: a) The wavelength of an x-ray is 1.00 x10 -9 m or 1 nm, what is the frequency of this x-ray? b) If the wavelength of Long wavelength electromagnetic radiation is 7.65 x 104 m, what is the frequency of this Long wavelength radiation used to contact submerged nuclear submarines at sea? Solution: frequency(s-1 or Hz) = speed of light (m/s) wavelength(m) frequency = = 3.00 x 1017 s-1 (Hz)3.00 x 10 8 m/s 1.00 x 10 - 9 m a) b) frequency = = 3.92 x 103 s-1 (Hz) 3.00 x 10 8 m/s 7.65 x 104 m Max Planck and Blackbody Radiation Blackbody radiation: When a solid object is heated, it emits light. If light is treated as a wave, one can show that E α 1/λ4 but that does not fit the observations. Planck proposed that light is only emitted as fixed quantities or quanta: E = nhν where h = 6.626 x 10-34 J s and n is an integer. Photoelectric Effect ¥ Since the threshold energy of Potassium is = 3.7 x 10 - 19 J, the red light will not have enough energy to knock an electron out of the potassium, but the blue light will eject an electron ! ¥ E Total = E Threshold + EKinetic Energy of Electron ¥ E Electron = ETotal - E Threshold ¥ E Electron = 5.0 x 10 - 19 J - 3.7 x 10 - 19 J = 1.3 x 10 - 19 J = hν ¥ and ν = 1.96 x 1014 Hz (infrared) The emission spectrum of hydrogen atoms The wavelengths observed are explained by: The Rydberg equation 1/λ = R(1/n12 - 1/n22) where R = 1.0968 x 107 m-1 and n = integers with n2 > n1 Niels Bohr proposed that hydrogen atoms only have certain fixed energy levels, which are associated with specific orbits. An atom can only absorb or emit a photon whose energy equals the difference between two energy states (orbits). Light and Atoms ¥ When an atom gains a photon, it enters an excited state. ¥ This state has too much energy - the atom must lose it and return back down to its ground state, the most stable state for the atom. ¥ An energy level diagram is used to represent these changes. Energy Level Diagram Light Emission Light Emission Light Emission Excited States photon’s path Ground State E Hydrogen atom energy states Bohr derived an equation for the energy of an electron in orbit using classical physics: E = - 2.18x10-18 J (Z2/n2) where n is an integer and Z is the charge of the nucleus. The emission spectrum for Hydrogen should be: ∆E = Efinal - Einitial = - 2.18x10-18 J (1/nf2 - 1/ni2) Since ∆E = hν = hc/λ, 1/λ = ∆E/hc, which gives: 1/λ = - 2.18x10-18 J (1/nf2 - 1/ni2) = 1.10x107 m (1/nf2 - 1/ni2) hc Emission Energetics Problem: A sodium vapor light street light emits bright yellow light of wavelength = 589 nm. What is the energy change for a sodium atom involved in this emission? How much energy is emitted per mole of sodium atoms? Solution: Ephoton = hν = = h x c λ ( 6.626 x 10 -34J s)( 3.00 x 10 8m/s) 589 x 10 -9m Ephoton = Eatom = 3.37 x 10 -19J/atom Energy per mole requires that we multiply by Avogadro s number. Emole = 3.37 x 10 -19J/atom x 6.022 x 1023 atoms/mole = Emole = 2.03 x 105 J/mol = 203 kJ / mol Emission Energetics Problem: A compact disc player uses light with a frequency of 3.85 x 1014 Hz. What is this light s wavelength? What portion of the electromagnetic spectrum does this wavelength fall? What is the energy of one mole of photons of this frequency? Solution: λ = c / ν = = 7.78 x 10 -7 m = 778 nm3.00 x 10 8m/s 3.85 x 1014/s 778 nm is in the Infrared region of the electromagnetic spectrum Ephoton = hν = (6.626 x 10 -34Js) x ( 3.85 x 1014 /s) = 2.55 x 10 -19 J Emole = (2.55 x 10 -19J) x (6.022 x 1023 / mole) = 1.54 x 105 J/mole Emission Energetics Problem: Find the energy change when an electron changes from the n=4 level to the n=2 level in the hydrogen atom? What is the wavelength of this photon? Solution: Ephoton = -2.18 x10 -18J - = 1 n12 1 n22 Ephoton = -2.18 x 10 -18J - = - 4.09 x 10 -19J 1 2 2 1 4 2 λ = = = h x c E (6.626 x 10 -34Js)( 3.00 x 108 m/s) 4.09 x 10 -19J λ = 4.87 x 10 -7 m = 487 nm The duality of matter Problems with the Bohr Model: ¥does not work for atoms with more than 1 electron ¥the classical physics predicts that the electron should rapidly crash into the nucleus Louis de Broglie: ¥reasoned that perhaps matter is wave-like ¥and that the electron is dimensionally restricted (i.e., a single or bit allows only certain wavelengths) ¥Since E = h¥c/λ = mc2, proposed that for any particle: λ = h/m¥u where u is the speed of a particle of mass u Quantum Numbers 2) Angular momentum quantum number (l ) ¥ is related to the sh ape of the orbital. ¥ Positive integer from 0 to ( n-1 ) ¥ n = 1 , l = 0; n = 2 , l = 0, 1; n = 3 , l = 0 , 1 , 2 Quantum Numbers 3) Magnetic Quantum Number - ml ¥ denotes the orientation of the orbital around the nucleus, describes the magnetic moment vector ¥ integers from -l through 0 to +l ¥ l = 0 , ml = 0; l =1 , ml = -1, 0, +1; l = 2 , ml = -2, -1, 0, +1, +2 Determining Quantum Numbers for an Energy Level Problem: What values of l and ml are allowed for a principal quantum number (n) of 4? How many orbitals are allowed for n = 4? Solution: The l values go from 0 to (n - 1), and for n = 4 they are: l = 0, 1, 2, 3. The values for ml go from -l to zero to +l For l = 0, ml = 0 l = 1, ml = -1, 0, +1 l = 2, ml = -2, -1, 0, +1, +2 l = 3, ml = -3, -2, -1, 0, +1, +2, +3 There are 16 ml values, so there are 16 orbitals for n=4 The total number of orbitals for a given value of n is n2, so for n = 4 there are 42 or 16 orbitals! l = 0 l = 1 l = 2 Energy Diagram of Orbitals (Approximate) l = 0 l = 1 l = 2 He Ne Ar Kr Xe Rn ZnCu Cd Hg Ag Au Ni Pd Pt Co Rh Ir Fe Ru Os Mn Tc Re Cr Mo W V Nb Ta Ti Zr Hf Sc Y La Ac The Periodic Table of the Elements S Orbita ls P Orbital s f Orbi tals Rf Ha Electronic Structure F Cl Br I At O S Se Te Po N P As Sb Bi C Si Ge Sn Pb B Al Ga In Tl H Li Be NaMg K Ca Rb Sr Cs Ba Fr Ra d Orbita ls Ce Pr Nd Sg PmSm EuGd Tb DyHo Er Tm Yb Lu Th Pa U Np PuAmCm Bk Cf Es FmMd NoLr
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