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Exam #3

Emma/Jace Wilson Inglês 59 flashcards

Exam #3

Flashcards do conjunto (59)

  1. 1Amplitudeheight of the wave, measured from the centerline between peak and trough
  2. 2Angular-Momentum Quantum Numberdefines the three-dimensional shape of the orbital
    If n=1, then l=0 If n=2, then l=0 or 1 If n=3, then l=0, 1, or 2… and so on
  3. 3Principal Quantum Number is Represented by what Character of the Alphabetn
  4. 4Angular-Momentum Quantum Number is Represented by what Character of the Alphabetl
  5. 5Aufbau Principleguides the filling order of orbitals
    (in general, each successive electron added to an atom occupies the lowest-energy orbital available)
  6. 6Balmer–Rydberg Equationm and n represent integers with n> m.Balmer–Rydberg Equation
  7. 7Balmer–Rydberg Equation: If m= ? then what? (m=1?, m=2?, m=3?)If m=1, then the ultraviolet series of lines results.
    If m=2, then Balmer’s series of visible lines results.
    If m=3, an infrared series is described, and so forth for still larger values of m.
  8. 8d-block elementmiddle of the table result from the filling of d orbitals
  9. 9de Broglie equationallows calculation of a “wavelength” of an electron or of any other particle or object of mass m moving at velocity v:
    λ=h/mv
  10. 10degenerateOrbitals that have the same energy level are degenerate
  11. 11Rules of the Aufbau Principle:1. Lower-energy orbitals fill before higher-energy orbitals.
    2. An orbital can hold only two electrons, which must have opposite spins.
    3. If two or more degenerate orbitals are available, one electron goes into each until all are half-full
  12. 12Hund's RuleIf two or more orbitals with the same energy are available, one electron goes in each until all are half full. The value of the spin quantum number of electrons in the half-filled orbitals will be the same.
  13. 13effective nuclear charge ZeffThe nuclear charge actually felt by an electron and is often substantially lower than the actual nuclear charge Z.
    Zeff = Zactual− Electron shielding
  14. 14Electromagnetic SpectrumThe spectrum consists of a continuous range of wavelengths and frequencies, from radio waves at the low-frequency end to gamma rays at the high-frequency end.
    Electromagnetic energy is characterized by a frequency, a wavelength, and an amplitude.
  15. 15Radiant EnergyAlthough they appear quite different to our senses, visible light, infrared radiation, microwaves, radio waves, X rays, and so on are all different forms of electromagnetic radiation
  16. 16electron configurationKnowing the relative energies of the various orbitals, we can predict for each element which orbitals are occupied by electrons—the element’s electron configuration
  17. 17f-block elementslanthanide/actinide f-block elements detached at the bottom of the table result from the filling of f orbitals.
  18. 18p-block elementsthe group 3A–8A elements on the right side of the table are the p-block elements because they result from the filling of p orbitals
  19. 19s-block elementsThe group 1A and group 2A elements on the left side of the table are called the s-block elements because they result from the filling of an s orbital
  20. 20Difference between: d-block f-block s-block p-blockDifference between: d-block f-block s-block p-block
  21. 21frequency (ν)a wave is simply the number of wave peaks that pass by a given point per unit time, usually expressed in units of reciprocal seconds, or hertz (Hz)
  22. 22wavelength (λ)the wave is the distance from one wave peak to the next
  23. 23Difference between.... Amplitude Wavelength FrequencyDifference between.... Amplitude Wavelength Frequency
  24. 24How do you calculate speed?How do you calculate speed?
  25. 25ground-state electron configurationlowest-energy configuration is called the ground-state electron configuration of the atom
  26. 26Heisenberg uncertainty principleIn 1927 by Werner Heisenberg (1901–1976) that it is impossible to know precisely where an electron is and what path it follows
    Heisenberg uncertainty principle.
    (Δx)(Δmv) ≥ h/4π
  27. 27hertz (Hz)units of reciprocal seconds
  28. 28line spectrum(White Light) When passed first through a narrow slit and then through a prism, the light emitted by an excited atom is found to consist of only a few wavelengths rather than a full rainbow of colors, giving a series of discrete lines on an otherwise dark background
  29. 29Example of Line SpectrumIf hydrogen atoms are electrically excited in a discharge tube, they give off a pinkish light made of several different colors
  30. 30magnetic quantum number (ml)defines the spatial orientation of the orbital with respect to a standard set of coordinate axes.
    For an orbital whose angular-momentum quantum number is l, the magnetic quantum number ml can have any integral value from −l to +l.
  31. 31nodea surface of zero electron probability separating regions of nonzero probability
  32. 32orbitalor wave functions
    a solution to the Schrödinger wave equation, describing a region of space where an electron is likely to be found
  33. 33Pauli exclusion principleNo two electrons in an atom can have the same four quantum numbers.
  34. 34phasea state of matter
  35. 35photonthe smallest possible amount of radiant energy; a quantum
  36. 36photoelectric effectthe ejection of electrons from metal on exposure to radiant energyphotoelectric effect
  37. 37Planck’s postulatethe energy of one quantum is related to the frequency of an electromagnetic wave
    Planck’s postulate E = hν = hc/λ
  38. 38quantumthe smallest possible amount of radiant energy
  39. 39quantizedmeaning that both matter and electromagnetic energy occur only in discrete amounts.
  40. 40quantum mechanical modela model of atomic structure that concentrates on an electron’s wavelike properties
    The fundamental idea behind the model is that it’s best to abandon the notion of an electron as a small particle moving around the nucleus in a defined path and to concentrate instead on the electron’s wavelike properties.
  41. 41quantum numberis a positive integer (n=1, 2, 3, 4,…) on which the size and energy level of the orbital primarily depends.
    For hydrogen and other one-electron atoms, such as He+, the energy of an orbital depends only on n.
    For atoms with more than one electron, the energy level of an orbital depends both on n and on the l quantum number.
  42. 42Rutherford’s nuclear modelan atom must consist mostly of empty space, having a dense, positively charged nucleus at its center
  43. 43shella grouping of orbitals according to the principal quantum number
  44. 44spin quantum numberElectrons behave in some ways as if they were tiny charged spheres spinning around an axis. This spin (blue arrow) gives rise to a tiny magnetic field (green arrow) and to a fourth quantum number, ms, which can have a value of either +1/2 or −1/2.spin quantum number
  45. 45subshella grouping of orbitals by angular-momentum quantum number
  46. 46valence shellthe outermost electron shell
    all the elements in a given group of the periodic table have similar valence-shell electron configurations
  47. 47wave functionor orbitals
    a solution to the Schrödinger wave equation
  48. 48Born–Haber cyclea pictorial way of viewing the energy changes in the various steps during formation of an ionic solid from its elements
  49. 49core electroninner-shell electrons
  50. 50Coulomb’s lawThe force resulting from the interaction of two electric charges is equal to a constant k times the magnitude of the charges divided by the square of the distance between them.
  51. 51electron affinity (Eea)the energy change that occurs when an electron is added to an isolated atom in the gaseous state
  52. 52ground-state electron configurationthe lowest-energy electron configuration of an atom
  53. 53ionic bondoccurs when one atom transfers an electron to another, creating an electrostatic attraction between positively charged cations and negatively charged anions
    A familiar example of an ionic compound is table salt, NaCl, consisting of Na+ and Cl− ions
  54. 54ionic solida solid whose constituent particles are ions ordered into a regular three– dimensional arrangement held together by ionic bonds
  55. 55ionization energy (Ei)the amount of energy necessary to remove the outermost electron from an isolated neutral atom in the gaseous state
  56. 56isoelectronicAtoms or ions with same electron configuration
    main group ions are isoelectronic to noble gases
  57. 57lattice energy (U)the sum of the electrostatic interactions between ions in a solid that must be overcome to break a crystal into individual ions
    amount of energy that must be added to break up an ionic solid into its individual gaseous ions, so it has a positive value
  58. 58octet ruleMain-group elements tend to undergo reactions that leave them with eight outer-shell electrons. That is, main-group elements react so that they attain a noble-gas electron configuration with filled s and p sublevels in their valence electron shell.
  59. 59shieldedValence electrons are strongly shielded by inner-shell (core) electrons. They are less strongly shielded by other electrons in the same shell and the magnitude of shielding follows the order: s>p>d>f.

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FlashCards sobre Exam #3, criado por Emma/Jace Wilson em 02-06-2019.
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