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45 Terms

1
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Thomas Young

  • examined one light source sent through two openings

  • observed constructive and destructive interference patterns

LIGHT IS A WAVE

2
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Wavelength

  • (lambda) is the distance between identical points on successive waves. (m or nm) (1m = 1 x 10^9nm)

3
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Frequency

  • (n) is the number of waves that pass through a particular point in 1 second (Hz = 1 cycle/s).

4
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Electromagnetic radiation

lambda x v = c

  • lambda = wavelength

  • v = frequency

  • c = speed of light = 3.00 × 10^8 m/s

5
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Electromagnetic Spectrum

  • Red Martians Invade Venus Using X-ray Guns

    • Visible Light: 400 nm - 700 nm

<ul><li><p>Red Martians Invade Venus Using X-ray Guns</p><ul><li><p>Visible Light: 400 nm - 700 nm</p></li></ul></li></ul><p></p>
6
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Planck

  • Heated Solids Problem

    • Solids emit electromagnetic radiation over a wide range of wavelengths when solids are heated. Radiant energy emitted by an object at a certain temperature corresponds to their wavelength and frequency

    • Energy(light) is emitted or absorbed in discrete units(quantum)

    • E = h x v

      • E: energy of a photon of light (J)

      • h = Planck’s constant = 6.63 × 10^-34 Jxs

      • v = frequency of light (1/s)

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Einstein

  • Photoelectric Effect(1905)

    • Light has both wave and particle nature

    • Photon is a “particle” of light

    • hv = KE + W

      • hv = energy of the photons of light hitting metal

      • W = work function

      • KE = energy of ejected electron

8
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Relationship between frequency and wavelength

Inversely proportional

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Relationship between frequency and energy

Directly proportional

10
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Hz in a GHZ

10^9

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nm in a m

1 × 10^9

12
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Bohrs Model of the Atom

  • Have quantized energy values(n=1, n=2, n=3…)

  • Able to jump to higher orbitals when they absorb enough energy

  • When electrons move towards nucleus, light is emitted and the energy is dependent on the energy difference

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Energy of jump

En = -Rh (1/n²)

E = - Rh (1/nf² - 1/2i²)

  • n = 1,2,3, …

  • Rh (Rydberg constant) = 2.18 × 10^-18 J

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Ion

  • An atom/group of atoms that has a net positive or negative charge due to the loss or gain of electrons

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Shell*

  • Area around the nucleus where electrons reside (n)

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Orbital

  • Specific area in the shell when the electrons reside

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Valence electrons

  • Electrons in the outermost shell

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Octet Rule

  • To be “happy” atoms want 8 valence electrons – LOW

    ENERGY (**Exception – the first shell only wants 2 electrons)

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Cation

  • Ion with a positive charge

  • Neutral atom loses one or more electrons

<ul><li><p>Ion with a positive charge</p></li><li><p>Neutral atom loses one or more electrons</p></li></ul><p></p>
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Anion

  • Ion with a negative charge

  • Neutral atom gains one or more electrons

  • ide

<ul><li><p>Ion with a negative charge</p></li><li><p>Neutral atom gains one or more electrons</p></li><li><p>ide</p></li></ul><p></p>
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Work function

  • How strong/tight electron is bound to the metal

22
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Emission Spectra

  • Charging gas in a tube which separates light into different components with a prism

23
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J in a Kj

1000J

24
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Shortcoming of Bohr

  • Didn’t account for emission spectra of atoms that have more than one electron

  • Conflict with wavelike properties

25
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Heisenberg Uncertainty Principle

  • Impossible to know the momentum p (m x v) and the position of a particle with certainty

26
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Schrodinger

  • Equation describes particle and wave nature of the e-

  • Hydrogen atom

  • Wave function(psy):

    • Energy of e- with a given psy

    • psy ² = probability of finding electron in a volume of space

27
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Electron density

  • Probability that an electron will be found in a particular region of an atom

28
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Atomic orbital

  • Probability of locating an electron in space

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Principal quantum number n

  • Distance of electron from the nucleus and average energy

  • n = 1, 2, 3, 4, …

30
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Angular momentum quantum number /

  • Shape of the atomic orbital

  • Orbitals

    • l = 0

    • l = 1

    • l = 2

    • l = 3

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Magnetic Quantum Number ml

  • Orientation of the orbital in space

32
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Spin quantum number ms

  • ms = -1/2 or +1/2

33
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Pauli exclusion principle

  • No two electrons in an atom can have the same four quantum numbers

<ul><li><p>No two electrons in an atom can have the same four quantum numbers</p></li></ul><p></p>
34
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Hunds Rule

  • The most stable arrangement of electrons in subshells is the one with the greatest number of parallel spins

35
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Aufbaus Principle

  • When in the ground state, electrons must fill orbitals from the lowest energy to the highest energy

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Shell

  • Electrons with the same value of n

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Subshell

  • Electrons with the same values of n and l

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Orbital

  • Electrons with the same values of n, l, and ml

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Total orbitals

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Total electrons

2n²

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Paramagnetic

  • When there are unpaired electrons that are attracted to external magnetic fields

<ul><li><p>When there are unpaired electrons that are attracted to external magnetic fields</p></li></ul><p></p>
42
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Diamagnetic

  • When electrons are paired

<ul><li><p>When electrons are paired</p></li></ul><p></p>
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Isoelectronic

  • Have the same number of electrons and the same ground-state electron configuration

44
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Constructive

  • Crest to crest - > Constructive Interference

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Destructive

  • Crest to trough → Destructive Interference