Chapter 3.1-3.2 Flashcards

1
Q

What is a wave?

A

Light behaves as a wave

You can calculate it

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Wave Characteristics

A

Speed of light (c): 2.998x10^8 m/s

Wavelength: the distance from one peak to the next

Frequency (v): is the number of wavelengths (“cycles”) that pass a point in a given period of time

Amplitude: 1/2 the height between peaks & throughs

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

electromagnetic spectrum

A

The electromagnetic spectrum is the range of frequencies of electromagnetic radiation and their respective wavelengths and photon energies.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

How do we know light acts as a wave?

A

a) Constructive interference

b) Destructive interference

Waves bend around and encounters an obstacle slit that is about the same size of the wavelength is diffreacts (think about a light curve under a closed door)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Diffraction Definition

A

The scattering of photon waves by an object such as an electron cloud, resulting in constructive or destructive interference

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Standing Waves

A

waves constrained in some particular region of space

-can have only a half-integer # of wavelengths

-Standing waves exhibit nodes: places where the amplitude remains zero

-As the energy increases, so does the # of wavelengths & the # of nodes

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Blackbody Radiation

A

-The emission of photons over a broad and continuous range of
wavelengths

Substances produce a continuous spectrum when heated
Objects array different temperatures

-As temp increases, total intensity increases, max wavelength increases

-1900 Max Planck proposed that the energy of light came in discreet “chunks”: light is quantized

h (Planck’s constant) = 6.626x10^-34

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Photoelectric Effect

A

-1902: Philip Kenard found three rules for the photoelectric effect

  1. No electrons are emitted unless the light has a frequency above a threshold, which varies for different metals
  2. Electrons are ejected immediately

Finish

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Einstein’s Explanation

A
  • Light energy was delivered to the atoms in packets called photons, with energy (E)
  • One photon at the threshold frequency has just enough energy for an electron to escape the atom
  • High frequencies: electron absorbs more energy, excess energy becomes kinetic energy of the ejected electron
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

The wave-particle Duality of Light

A

Light behaves like both a wave..
-has a speed, wavelength, frequency
-exhibits interference and diffraction

… and like a particle

-blackbody radiation, Finish

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Line spectra

A

-When atoms absorb energy (heat, electrical current),
that energy is often released as light

-When that light is passed through a prism, a pattern is seen that is unique to that type of atom: atomic emission spectrum

-The light is emitted only at a few specific wavelengths: line source or line spectrum

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

Atom spectrum of Hydrogen

A
  • 1885: Balmer noted that wavelengths of the lines in the visible spectrum of hydrogen followed by a simple formula

-1888: Rydberg created a general equation for the wavelengths of the line spectrum of hydrogen: Rydberg equation:

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Bohr Model of the Atom

A

1

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Wavelength as it relates to a electromagnetic

A

Wavelength is the distance between two consecutive peaks or troughs in a wave

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

Color of light, frequency and wave length

A

Red light has a lower frequency and a longer wavelength than ultraviolet rays.

Ultraviolet rays has a higher frequency and a shorter wavelength than red light.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Symbols and equations:

A

The speed of a wave (c)
frequency ν
wavelength λ
energy of a photon equals its Planck’s constant (h)

c=λν

E=photon energy

h=pats constant

E = hv

17
Q
A

The energy (E) of a photon of light is proportional to its frequency (ν) or the inverse of its wavelength (λ) multiplied by Planck’s constant (h):

E=hu=hc/λ
As such, light with a lot of energy will have a high frequency and a small wavelength.

18
Q

Bohr Model

A
  1. The energy of the electron was
    proportional the distance the orbit
    was from the nucleus: energy of
    electron is quantized
  2. The atom emitted a photon when the electron “jumped” from an orbit
    with higher energy down to an orbit with lower energy
  3. If the atom absorbed a photon of a certain freq., the electron “jumped”
    from an orbit with lower energy to an orbit with higher energy
19
Q

How does the Bohr Model work?

A

When an electron jumps among diff. orbits, energy is emitted or absorbed as photons✓ from larger n to smaller n: photon emission
✓ opposite is photon absorption
✓ n is the principal quantum number
✓ Joule (J) is the SI unit for energy
➢ 1 J = 1 kg m2/s2

20
Q

Bohrs model and Liberge equation

A

Bohrs model finds the awnser to the Liberge equation:

21
Q

What falts does the Bohr Model have?

A
  1. It violates basic laws of physics (an electrically charged
    particle orbiting in a circular path should lose energy, so the
    electron should eventually spiral into the nucleus)
  2. It fails to explain the line spectra of any elements other than
    hydrogen
22
Q

What new Ideas did the Bohr Model introduce?

A

Nonetheless, the Bohr model introduced some key ideas:
1. Energies of electrons in atoms are quantized, given by
quantum numbers
2. An electron’s energy increases with increasing quantum
number and thus distance from the nucleus
3. The discreet line spectra of elements result from transitions
between these quantized electronic energy levels of atoms

23
Q

Wave Nature of Matter

A

1925: de Broglie proposed that electrons (like photons) were both particles & waves
✓ de Broglie wavelength

• 1927: Davisson and Germer showed that electrons exhibit diffraction

  • De Broglie said the electroons were standing waves
24
Q
A

When you try to observe a photons location it starts to act like a partical instead of a wave

25
Q

Heisenberg’s Uncertainty Principle

A

1927: Heisenberg’s uncertainty principle: “If a measurement of position is made with precision x and a simultaneous measurement of momentum is made with precision p, then the product of the 2 uncertainties must be ≥ h/4p.”

• This has nothing to do w/ imperfections in our measurement abilities: it

26
Q

Does the orbital in the bohr model impact the energy level

A

The higher the orbital the higher the energy level

27
Q

work function

A

is the energy that must be supplied to cause the release of an electron from a photoelectric material. The corresponding photon frequency is the threshold frequency. The higher the energy of the incident light, the more kinetic energy the electrons have in moving away from the surface.

28
Q

What does ψ² discribe?

A

While the wave function ψ describes the overall state of a quantum system, the square of the wavefunction (ψ2) gives the probability of finding an electron in a given region of space.

29
Q

Memorize

A

Atomic orbitals are described by their principal quantum number (n) followed by a letter that corresponds to the value for the angular momentum quantum number (ℓ). Here, n= 3, so the atomic orbital symbol will begin with 3. The quantum number p = 1 (s = 0, p = 1, d = 2, f = 3), which corresponds to p. Therefore, this is a 3p atomic orbital.