logging in or signing up Atomic Structure nade992 Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINT lite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 432 Category: Entertainment License: All Rights Reserved Like it (2) Dislike it (0) Added: April 26, 2010 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... By: kevin_patel (18 month(s) ago) download unavailable what is the use of it if you are not allowing others to see your creativity Saving..... Post Reply Close Saving..... Edit Comment Close By: neerajguglani12 (24 month(s) ago) Nice Atomic structure Saving..... Post Reply Close Saving..... Edit Comment Close Premium member Presentation Transcript Slide 1: Atomic Structure Slide 2: All waves have a characteristic wavelength, l, and amplitude, A. Frequency, n, of a wave is the number of cycles which pass a point in one second. Speed of a wave, c, is given by its frequency multiplied by its wavelength: For light, speed = c = 3.00x108 m s-1 . A Brief History of Time The Wave Nature of Light Slide 3: The Wave Nature of Light Slide 4: The Wave Nature of Light Slide 5: The Wave Nature of Light Slide 6: Planck: energy can only be absorbed or released from atoms in certain amounts called quanta. The relationship between energy and frequency is where h is Planck’s constant ( 6.626 10-34 J s ) . Quantized Energy and Photons Slide 7: The Photoelectric Effect and Photons Einstein assumed that light traveled in energy packets called photons. The energy of one photon is: Quantized Energy and Photons Slide 8: Nature of Waves: Quantized Energy and Photons Slide 9: Line Spectra Radiation composed of only one wavelength is called monochromatic. Radiation that spans a whole array of different wavelengths is called continuous. White light can be separated into a continuous spectrum of colors. Note that there are no dark spots on the continuous spectrum that would correspond to different lines. Line Spectra and the Bohr Model Slide 11: Bohr Model Colors from excited gases arise because electrons move between energy states in the atom. (Electronic Transition) Line Spectra and the Bohr Model Slide 12: Bohr Model Since the energy states are quantized, the light emitted from excited atoms must be quantized and appear as line spectra. After lots of math, Bohr showed that where n is the principal quantum number (i.e., n = 1, 2, 3, … and nothing else). Line Spectra and the Bohr Model Slide 13: Bohr Model We can show that When ni > nf, energy is emitted. When nf > ni, energy is absorbed Line Spectra and the Bohr Model Slide 14: Bohr Model Line Spectra and the Bohr Model CyberChem (Fireworks) video Mathcad (Balmer Series) Slide 15: Line Spectra and the Bohr Model: Balmer Series Calculations Slide 17: Limitations of the Bohr Model Can only explain the line spectrum of hydrogen adequately. Can only work for (at least) one electron atoms. Cannot explain multi-lines with each color. Electrons are not completely described as small particles. Electrons can have both wave and particle properties. Line Spectra and the Bohr Model Slide 18: Knowing that light has a particle nature, it seems reasonable to ask if matter has a wave nature. Using Einstein’s and Planck’s equations, de Broglie showed: The momentum, mv, is a particle property, whereas is a wave property. de Broglie summarized the concepts of waves and particles, with noticeable effects if the objects are small. The Wave Behavior of Matter Slide 19: The Uncertainty Principle Heisenberg’s Uncertainty Principle: on the mass scale of atomic particles, we cannot determine exactly the position, direction of motion, and speed simultaneously. For electrons: we cannot determine their momentum and position simultaneously. If Dx is the uncertainty in position and Dmv is the uncertainty in momentum, then The Wave Behavior of Matter Energy and Matter : Energy and Matter E = m c2 Slide 21: Schrödinger proposed an equation that contains both wave and particle terms. Solving the equation leads to wave functions. The wave function gives the shape of the electronic orbital. [“Shape” really refers to density of electronic charges.] The square of the wave function, gives the probability of finding the electron ( electron density ). Quantum Mechanics and Atomic Orbitals Slide 22: Quantum Mechanics and Atomic Orbitals Solving Schrodinger’s Equation gives rise to ‘Orbitals.’ These orbitals provide the electron density distributed about the nucleus. Orbitals are described by quantum numbers. Slide 23: Orbitals and Quantum Numbers Schrödinger’s equation requires 3 quantum numbers: Principal Quantum Number, n. This is the same as Bohr’s n. As n becomes larger, the atom becomes larger and the electron is further from the nucleus. ( n = 1 , 2 , 3 , 4 , …. ) Azimuthal Quantum Number, . This quantum number depends on the value of n. The values of begin at 0 and increase to (n - 1). We usually use letters for (s, p, d and f for = 0, 1, 2, and 3). Usually we refer to the s, p, d and f-orbitals. Magnetic Quantum Number, m. This quantum number depends on . The magnetic quantum number has integral values between - and + . Magnetic quantum numbers give the 3D orientation of each orbital. Quantum Mechanics and Atomic Orbitals Quantum Numbers of Wavefuntions : Quantum Numbers of Wavefuntions Quantum Mechanics and Atomic Orbitals : Quantum Mechanics and Atomic Orbitals Slide 26: Orbitals and Quantum Numbers Quantum Mechanics and Atomic Orbitals Slide 27: The s-Orbitals Representations of Orbitals Slide 28: The p-Orbitals Representations of Orbitals Slide 29: d-orbitals Slide 30: Many-Electron Atoms Orbitals and Their Energies Orbitals CD Slide 31: Electron Spin and the Pauli Exclusion Principle Many-Electron Atoms Slide 32: Electron Spin and the Pauli Exclusion Principle Since electron spin is quantized, we define ms = spin quantum number = ½. Pauli’s Exclusions Principle: no two electrons can have the same set of 4 quantum numbers. Therefore, two electrons in the same orbital must have opposite spins. Many-Electron Atoms Slide 33: Figure 6.27 Figure 6.27 Orbitals CD Slide 34: Figure 6.28 Orbitals CD Slide 35: Many-Electron Atoms Orbitals and Their Energies Orbitals CD Slide 36: Electron Configurations Slide 37: Metals, Nonmetals, and Metalloids Metals Figure 7.14 Slide 38: Two Major Factors: principal quantum number, n, and the effective nuclear charge, Zeff. Periodic Trends Slide 39: Figure 7.5: Radius video Clip Slide 40: Figure 7.6 Slide 41: Figure 7.10 IE clip Slide 42: Figure 7.9 Slide 43: Electron Affinities Electron affinity is the opposite of ionization energy. Electron affinity: the energy change when a gaseous atom gains an electron to form a gaseous ion: Cl(g) + e- Cl-(g) Electron affinity can either be exothermic (as the above example) or endothermic: Ar(g) + e- Ar-(g) Slide 44: Figure 7.11: Electron Affinities Slide 45: Group Trends for the Active Metals Group 1A: The Alkali Metals Slide 46: Group Trends for the Active Metals Group 2A: The Alkaline Earth Metals Slide 47: Group Trends for Selected Nonmetals Group 6A: The Oxygen Group Slide 48: Group Trends for Selected Nonmetals Group 7A: The Halogens Slide 49: Group Trends for the Active Metals Group 1A: The Alkali Metals Alkali metals are all soft. Chemistry dominated by the loss of their single s electron: M M+ + e- Reactivity increases as we move down the group. Alkali metals react with water to form MOH and hydrogen gas: 2M(s) + 2H2O(l) 2MOH(aq) + H2(g) Slide 50: Group Trends for the Active Metals Group 2A: The Alkaline Earth Metals Alkaline earth metals are harder and more dense than the alkali metals. The chemistry is dominated by the loss of two s electrons: M M2+ + 2e-. Mg(s) + Cl2(g) MgCl2(s) 2Mg(s) + O2(g) 2MgO(s) Be does not react with water. Mg will only react with steam. Ca onwards: Ca(s) + 2H2O(l) Ca(OH)2(aq) + H2(g) Slide 51: Atomic Structure You do not have the permission to view this presentation. In order to view it, please contact the author of the presentation.
Atomic Structure nade992 Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINT lite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 432 Category: Entertainment License: All Rights Reserved Like it (2) Dislike it (0) Added: April 26, 2010 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... By: kevin_patel (18 month(s) ago) download unavailable what is the use of it if you are not allowing others to see your creativity Saving..... Post Reply Close Saving..... Edit Comment Close By: neerajguglani12 (24 month(s) ago) Nice Atomic structure Saving..... Post Reply Close Saving..... Edit Comment Close Premium member Presentation Transcript Slide 1: Atomic Structure Slide 2: All waves have a characteristic wavelength, l, and amplitude, A. Frequency, n, of a wave is the number of cycles which pass a point in one second. Speed of a wave, c, is given by its frequency multiplied by its wavelength: For light, speed = c = 3.00x108 m s-1 . A Brief History of Time The Wave Nature of Light Slide 3: The Wave Nature of Light Slide 4: The Wave Nature of Light Slide 5: The Wave Nature of Light Slide 6: Planck: energy can only be absorbed or released from atoms in certain amounts called quanta. The relationship between energy and frequency is where h is Planck’s constant ( 6.626 10-34 J s ) . Quantized Energy and Photons Slide 7: The Photoelectric Effect and Photons Einstein assumed that light traveled in energy packets called photons. The energy of one photon is: Quantized Energy and Photons Slide 8: Nature of Waves: Quantized Energy and Photons Slide 9: Line Spectra Radiation composed of only one wavelength is called monochromatic. Radiation that spans a whole array of different wavelengths is called continuous. White light can be separated into a continuous spectrum of colors. Note that there are no dark spots on the continuous spectrum that would correspond to different lines. Line Spectra and the Bohr Model Slide 11: Bohr Model Colors from excited gases arise because electrons move between energy states in the atom. (Electronic Transition) Line Spectra and the Bohr Model Slide 12: Bohr Model Since the energy states are quantized, the light emitted from excited atoms must be quantized and appear as line spectra. After lots of math, Bohr showed that where n is the principal quantum number (i.e., n = 1, 2, 3, … and nothing else). Line Spectra and the Bohr Model Slide 13: Bohr Model We can show that When ni > nf, energy is emitted. When nf > ni, energy is absorbed Line Spectra and the Bohr Model Slide 14: Bohr Model Line Spectra and the Bohr Model CyberChem (Fireworks) video Mathcad (Balmer Series) Slide 15: Line Spectra and the Bohr Model: Balmer Series Calculations Slide 17: Limitations of the Bohr Model Can only explain the line spectrum of hydrogen adequately. Can only work for (at least) one electron atoms. Cannot explain multi-lines with each color. Electrons are not completely described as small particles. Electrons can have both wave and particle properties. Line Spectra and the Bohr Model Slide 18: Knowing that light has a particle nature, it seems reasonable to ask if matter has a wave nature. Using Einstein’s and Planck’s equations, de Broglie showed: The momentum, mv, is a particle property, whereas is a wave property. de Broglie summarized the concepts of waves and particles, with noticeable effects if the objects are small. The Wave Behavior of Matter Slide 19: The Uncertainty Principle Heisenberg’s Uncertainty Principle: on the mass scale of atomic particles, we cannot determine exactly the position, direction of motion, and speed simultaneously. For electrons: we cannot determine their momentum and position simultaneously. If Dx is the uncertainty in position and Dmv is the uncertainty in momentum, then The Wave Behavior of Matter Energy and Matter : Energy and Matter E = m c2 Slide 21: Schrödinger proposed an equation that contains both wave and particle terms. Solving the equation leads to wave functions. The wave function gives the shape of the electronic orbital. [“Shape” really refers to density of electronic charges.] The square of the wave function, gives the probability of finding the electron ( electron density ). Quantum Mechanics and Atomic Orbitals Slide 22: Quantum Mechanics and Atomic Orbitals Solving Schrodinger’s Equation gives rise to ‘Orbitals.’ These orbitals provide the electron density distributed about the nucleus. Orbitals are described by quantum numbers. Slide 23: Orbitals and Quantum Numbers Schrödinger’s equation requires 3 quantum numbers: Principal Quantum Number, n. This is the same as Bohr’s n. As n becomes larger, the atom becomes larger and the electron is further from the nucleus. ( n = 1 , 2 , 3 , 4 , …. ) Azimuthal Quantum Number, . This quantum number depends on the value of n. The values of begin at 0 and increase to (n - 1). We usually use letters for (s, p, d and f for = 0, 1, 2, and 3). Usually we refer to the s, p, d and f-orbitals. Magnetic Quantum Number, m. This quantum number depends on . The magnetic quantum number has integral values between - and + . Magnetic quantum numbers give the 3D orientation of each orbital. Quantum Mechanics and Atomic Orbitals Quantum Numbers of Wavefuntions : Quantum Numbers of Wavefuntions Quantum Mechanics and Atomic Orbitals : Quantum Mechanics and Atomic Orbitals Slide 26: Orbitals and Quantum Numbers Quantum Mechanics and Atomic Orbitals Slide 27: The s-Orbitals Representations of Orbitals Slide 28: The p-Orbitals Representations of Orbitals Slide 29: d-orbitals Slide 30: Many-Electron Atoms Orbitals and Their Energies Orbitals CD Slide 31: Electron Spin and the Pauli Exclusion Principle Many-Electron Atoms Slide 32: Electron Spin and the Pauli Exclusion Principle Since electron spin is quantized, we define ms = spin quantum number = ½. Pauli’s Exclusions Principle: no two electrons can have the same set of 4 quantum numbers. Therefore, two electrons in the same orbital must have opposite spins. Many-Electron Atoms Slide 33: Figure 6.27 Figure 6.27 Orbitals CD Slide 34: Figure 6.28 Orbitals CD Slide 35: Many-Electron Atoms Orbitals and Their Energies Orbitals CD Slide 36: Electron Configurations Slide 37: Metals, Nonmetals, and Metalloids Metals Figure 7.14 Slide 38: Two Major Factors: principal quantum number, n, and the effective nuclear charge, Zeff. Periodic Trends Slide 39: Figure 7.5: Radius video Clip Slide 40: Figure 7.6 Slide 41: Figure 7.10 IE clip Slide 42: Figure 7.9 Slide 43: Electron Affinities Electron affinity is the opposite of ionization energy. Electron affinity: the energy change when a gaseous atom gains an electron to form a gaseous ion: Cl(g) + e- Cl-(g) Electron affinity can either be exothermic (as the above example) or endothermic: Ar(g) + e- Ar-(g) Slide 44: Figure 7.11: Electron Affinities Slide 45: Group Trends for the Active Metals Group 1A: The Alkali Metals Slide 46: Group Trends for the Active Metals Group 2A: The Alkaline Earth Metals Slide 47: Group Trends for Selected Nonmetals Group 6A: The Oxygen Group Slide 48: Group Trends for Selected Nonmetals Group 7A: The Halogens Slide 49: Group Trends for the Active Metals Group 1A: The Alkali Metals Alkali metals are all soft. Chemistry dominated by the loss of their single s electron: M M+ + e- Reactivity increases as we move down the group. Alkali metals react with water to form MOH and hydrogen gas: 2M(s) + 2H2O(l) 2MOH(aq) + H2(g) Slide 50: Group Trends for the Active Metals Group 2A: The Alkaline Earth Metals Alkaline earth metals are harder and more dense than the alkali metals. The chemistry is dominated by the loss of two s electrons: M M2+ + 2e-. Mg(s) + Cl2(g) MgCl2(s) 2Mg(s) + O2(g) 2MgO(s) Be does not react with water. Mg will only react with steam. Ca onwards: Ca(s) + 2H2O(l) Ca(OH)2(aq) + H2(g) Slide 51: Atomic Structure