Atoms Flashcards

You may prefer our related Brainscape-certified flashcards:
1
Q

graph of scattering angle with no. of α particles scattered

A

kind of like inversely proportional

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

Significance of α particle experiment

A

Most of them passed undeflected
Most space of atom is empty
Few deflected through 90 & 180
All +ve charge & the mass of atom is concentrated in a very small region called nucleus
Size of nucleus is 1/10^15m & that of atom is 1/10^10m
Since gold nucleus is much heavier than α particle, gold nucleus remains at rest

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

Impact parameter

A

Perpendicular distance of initial velocity vector of α particle from center of nucleus

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

For large impact parameter, α particle is

A

almost undeflected

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

For head on collision, impact parameter is

A

0

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

Rutherford’s postulates

A

Entire +ve charge & mass of atom is concentrated at very small volume at the center called nucleus
Amount of +ve charge is equal to -ve charge
Atom is neutral
E’s are continuously revolving around the nucleus in circular orbits
Force of attraction provides necessary centripetal force

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

Limitations of Rutherford’s atomic model

A
  1. an accelerating particle emits radiation as EM waves. So energy of the electron show gradually decrease leading to decrease in radius of e’ orbit
  2. Electron follows a spiral path & finally fall into the nucleus so atom isn’t stable
  3. As e’ spiral inwards, their angular velocity & their freq change continuously they would emit continuous spectrum instead of actually observed line spectrum
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Bohr’s atomic model

A
  1. In a H atom, an e’ revolves in stable orbits called stationary orbits
  2. These orbits are those for which angular momentum is integral multiple of h/2pi
    As long as e’ is revolving in stationary orbit, it doesn’t radiate energy. When e’ make a transition from higher energy to lower, a photon is emitted, having energy equal to energy diff b/n initial & final states
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

radius of orbit r =

A

n²h²ε/Ze²pi m

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Are stationary orbits equally spaced?

A

No

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

Speed _______ as we move away from the nucleus

A

decreases

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

Potential energy U =

A

-kZe²/r

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

Kinetic energy K =

A

kZe²/2r

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

E =

A

-mZ²e⁴/8ε²n²h²

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

-ve sign in E indicates that?

A

e’ is bound to nucleus so energy is needed to be done to separate e’ from nucleus

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

Rydberg const

A

1.1 x 10⁷ per metre

17
Q

For lyman series, n2 =

A

2,3,4,….

18
Q

Lyman series lies in

A

UV region

19
Q

Balmer region lies in

A

1st 4 lines in visible region and later in UV

20
Q

For alpha H, n1 & n2 =

A

2; 3

21
Q

For beta H, n1 & n2 =

A

2; 4

22
Q

Paschen and Pfund lies in

A

IR region

23
Q

Excitation energy of atom

A

Energy required by an e’ to jump from the ground state to any one of excited states

24
Q

Ionisation energy

A

Energy required to knock an e’ completely out of atom

25
Q

Limitations of Bohr’s model

A
  1. Capable only to H like atoms
  2. Couldn’t explain fine structure of spectral lines
  3. Doesn’t explain why only circular orbits are chosen where elliptical orbits are possible
  4. Doesn’t tell anything about relative intensities of various spectral lines
  5. Fails to explain further splitting of spectral lines in M.F & E.F
26
Q

Zeeman effect

A

Splitting of spectral lines in M.F

27
Q

Stark effect

A

Splitting of spectral lines in E.F

28
Q

Alpha particle has _________ penetrating power

A

least

29
Q

Lyman in ___ range

A

UV

30
Q

Balmer in ____ range

A

visible

31
Q

Paschen, Brackett, Pfund in ___ range

A

Infra Red