Atoms Flashcards

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1
Q

alpha particle scattering experiment - observations

A
  1. Most of the alpha particles pass through without appreciable deflection.
  2. Number of alpha particles scattered decreases sharply with angle of scattering
  3. Only very few (1 out of 10000) suffer 180-degree deflection.
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2
Q

alpha particle scattering experiment - conclusions

A
  1. Most part of the atom is empty space
  2. Most mass of the atom is concentrated in a small space.
  3. The positive charge of the atom along with the mass is concentrated into a small space called nucleus.
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3
Q

distance of closest approach (d) =

A

(1/4πε)×(2Ze^2/KE)

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4
Q

Define Impact Parameter.

A

Impact parameter is defined as the perpendicular distance between the initial velocity vector of the alpha particle and the line passing through the center of nucleus.

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5
Q

Expressions for potential, kinetic and total energy based on rutherford’s model.

A

PE = (1/4πε)×(-e^2/r)
KE = (1/8πε)×(e^2/r)
Total energy = -(1/8πε)×(e^2/r)

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6
Q

Two limitations of Rutherford’s model

A
  1. Could not explain the stability of atom as electrons revolving around the nucleus are supposed to radiate energy in the form of electromagnetic waves, as the energy decreases, the electrons are supposed to spiral into the nucleus and collapse but practically atoms are stable.
  2. Could not explain the line spectra of hydrogen atoms (could only explain continuous spectra). Since the electron spiral with continuously increasing frequency, it is supposed to emit only continuous spectrum of radiations.
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7
Q

The 1st postulate of Bohr’s model of an atom

A

Electrons around the nucleus can continue revolving without radiating energy in certain specified orbits known as non-radiating orbits or stable orbits.

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8
Q

The 2nd postulate of Bohr’s model of an atom

A

Electrons whose angular momentum is an integral multiple of h/2π can revolve without radiating energy.

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9
Q

The 3rd postulate of Bohr’s model of an atom

A

Electrons deexciting from higher energy level to lower energy level radiate energy equal to the difference in the energy levels of initial and final orbits.

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10
Q

Expressions for potential, kinetic and total energy according to Bohr’s model

A
PE =  (1/4πε)×(-me^4/n^2×h^2)
KE =  (1/8πε)×(me^e4/n^2×h^2)
TE =  -(1/8πε)×(me^4/n^2×h^2)
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11
Q

Expression for wavelength of photon emitted due to deexcitation of electron

A

1/λ = R((1/nf^2) - (1/ni^2))

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12
Q

for an electron to show stationary wave pattern, the circumference of the orbit =

A

nλ (where λ is the wavelength of electron in nth orbit/debroglie’s wavelength)

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13
Q

Debroglie’s wavelength =

A

h/mv

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14
Q

Limitations of Bohr’s Model

A
  1. Bohr failed to explain the splitting of spectral lines in magnetic field (Zeimann effect) and electric field (Stark effect).
  2. Bohr’s model was applicable only for hydrogen atom.
  3. Bohr failed to explain the relative intensity of different spectral lines.
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15
Q

number of spectral lines emitted when an electron undergo deexcitation from level n =

A

n(n-1)/ 2

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16
Q

hydrogen spectrum, n = 1

A

Lymann series
UV region
E1 = -13.6 eV

17
Q

hydrogen spectrum, n = 2

A

Balmer series
Visible region
E2 = -3.4 eV

18
Q

hydrogen spectrum, n = 3

A

Paschen series
Infrared region
E3 = -1.51 eV

19
Q

hydrogen spectrum, n = 4

A

Brackett series
Infrared region
E4 = -0.85 eV

20
Q

hydrogen spectrum, n = 5

A

Pfund series
Infrared region
E5 = -0.54 eV