Modern Physics lesson 1 (Black body Radiation) theory Flashcards

1
Q

after the discovery of phenomenon of what did they prove that light is a electromagnetic wave

A

interference, diffraction, polarization

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

it was assumed that light consists of tiny minute particles called

A

corpuscles

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

tell me about the emission and absorption of energy

A

emission and absorption of energy is not continuous, but discrete.

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

what are matter waves

A

A particle in motion is associated with waves called matter waves.

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

when is the object perfectly black XD

A

A perfect black body is the one which absorbs the entire radiations incident on
it, it neither reflects nor transmits radiations, and hence it appears perfectly
black

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

what happens when you heat a black body

A

it radiates all kind of wavelengths

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

The black body radiation is characteristic of its

A

temperature

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

What are radiation curves?

A

when a graph of energy density is plotted against wavelength, curves are obtained as
shown in the figure.

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

What are following conclusions can be drawn from the radiation curves.

A

1) The energy is not uniformly distributed in the spectrum of black body
radiation.
2) At a given temperature, energy density increases with wave length,
becomes maximum for a particular wavelength and then decreases as
wavelength increases.
3) As temperature increases, intense radiation represented by peak of the
curve shifts towards shorter wavelength region.

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

How many Laws of black body radiation are there

A

Stefan’s law of Radiation
Wein’s law of energy distribution
jean’s law of energy distribution
Planck’s law of radiation

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

What is Stefan’s law of radiation?

A

The Stefan’s law states that energy radiated per second per unit area is directly proportional to the fourth power of absolute temperature…..E directly proportional T 4, or E = σ T^4

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

What is Wien’s law of radiation?

A

Wien assumed that black body radiation in a cavity is supposed to be emitted by resonators of molecular dimensions having
Maxwellian velocity distribution and applied law of kinetic theory of gases to
obtain formula for energy distribution
Uλdλ=C1λ^-5e^[-(C2/λT)dλ

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

Drawbacks of Wien’s Law

A

This law explains the energy distribution only in shorter wavelengths & fails to
explain the energy distribution in longer wavelength region
when temperature is zero, energy density is finite. This is a contradiction to Stefan’s law

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

What is Lord Rayleigh –Jeans law of Radiation

A

Lord Rayleigh–Jeans considered the black body radiations full of electromagnetic
waves of all wavelengths, between 0 and infinity, which due to reflection, form
standing waves.
They calculated number of possible waves having wavelengths
between λand λ+dλ and by using law of equi-partition of energy, they established
distribution law as: Uλdλ=8πkT^-4dλ
Because of the presence of the factor t-4 in the equation, the energy radiated by the black body should rapidly decrease with
increasing wavelength.

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

Drawbacks of Rayleigh–Jeans law

A

Lord Rayleigh–Jeans law holds good only for longer wavelengths region and fails to explain energy distribution in shorter wavelength region,
The failure of the Rayleigh–Jeans law to explain the aspect of very little emission of radiation beyond the violet region towards the lower wavelength side of the spectrum is particularly referred to as Ultra-violet
Catastrophe.

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

Planck’s Law of Radiation

A

1) The black body radiations in a cavity are composed of tiny oscillators having molecular dimensions, which can vibrate with all possible frequencies.
2) The frequency of radiations emitted by oscillators is same as the frequency of its vibrations.
3) An oscillator cannot emit energy in a continuous manner, but emission
and absorption can take place only in terms of small packet of energy called Quanta, the oscillator can have only discrete energy values E given by nh ν

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

explain Compton scattering and Compton Effect.

A

Compton discovered that when monochromatic beam of very
high frequency radiation such as X-rays or Gamma rays is made to scatter
through a substance
the scattered radiation found to contain two components one having same frequency or wavelength as that of incident radiation, known as unmodified radiation
the other, having lower frequency or longer
wavelength than incident radiation known as modified radiation. This is called
Compton scattering
during the process an electron recoils with certain velocity. This phenomenon is called Compton Effect.

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

What is modified radiation

A

the scattered radiation having lower frequency or longer wavelength than incident radiation known as modified radiation

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

What is unmodified radiation

A

the scattered radiation one having same frequency or wavelength as that of incident radiation, known as unmodified radiation

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

What is Quanta or photons

A

radiation is composed of small packets of energy called Quanta or photons having energy hv

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

explain how the change in wavelength takes place during Compton effect

A

*According to Compton, when a
photon of energy hv of momentum h/λ moving with velocity equal to velocity of
light, obeying laws of conservation of energy and momentum, strikes an
electron which is at rest, there occurs an elastic collision between two particles
namely photon and electron
*When photon of energy h strikes the electron at rest, photon transfers some of
its energy to electron, therefore photon loses its energy, hence, its frequency
reduces to v1 and wavelength changes to λ1
* the scattered photon makes an
angle phi with the incident direction, during the process an electron gains kinetic
energy and recoils with certain velocity.
*by applying laws of conservation of energy and momentum we get
λ’-λ=h(1-cosphi)/m0c…..mo = mass of electron at rest

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

the change in wavelength (Compton shift) depends on?

A

thechange in wavelength (Compton shift) depends neither on the incident
wavelength nor the scattering material, but depends only on the angle of scattering

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

What is Compton shift.

A

The change in wavelength λ’-λ is called Compton shift

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

When the angle of scattering is 90o, the Compton shift is found to be

A

0.0243 A

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

What is the Physical significance of Compton Effect

A

*The phenomena of Compton effect is explained by Compton on the basis of
Quantum theory of radiation, in which it is assumed that radiation is composed
of small packets of energy called Quanta
*The Compton Effect is an elastic
collision between two particles namely photon and electron in which exchange
of energy takes place as if it is a particle–particle collision
* it is assumed that photon and electron obey laws of conservation of energy and momentum.
Hence Compton Effect signifies particle nature of radiation.

12
Q

what is the diff between a particle and a wave

A

*The concept of particle is easy to understand, because it has mass and occupies certain fixed position in space and particle in motion has definite momentum; when slowed down, it gives out energy. Therefore particle is specified by its mass, momentum, energy and position
*The concept of wave is bit difficult to understand, because a wave is a
disturbance spread over a large area. We cannot say wave is coming from here
or going there. No mass is associated with wave and the wave is characterized
by its wavelength, frequency, amplitude and phase.

13
Q

why is dual nature of both wave and particle accpeted

A

the phenomenon like interference and diffraction has shown beyond doubt the wave nature of light radiation
Huygens wave theory of light, however, experimental phenomenon like Photo electric effect, Compton Effect

13
Q

Explain De-Broglie concept of matter waves

A

According to this concept the dual characteristics of radiation is not confined
only to electromagnetic waves, but also holds good for all material particles in
motion i.e. all the particles like electrons, protons, neutrons, molecules, atoms
etc. exhibit dual characteristics
According to de-Broglie the particle in motion is associated with a group of
waves and controlled by the wave. This wave is known as matter wave or de
Broglie wave and wavelength associated with it is called de Broglie wavelength.

14
Q

Characteristics of Matter Waves

A
  • Matter waves are the waves associated with a moving particle.
  • The lighter the particle larger the wavelength.
  • Smaller the velocity of particle larger the wavelength.
  • The amplitude of the matter wave at a given point determines the
    probability of finding the particle at that point at a given instant of time.
  • The wavelength of a particle is given by, λ= h/p = h/mv
14
Q

what is Phase velocity or wave velocity

A

If a point is imagined to be marked on a travelling wave, then it becomes a representative point for a particular phase of the wave and the velocity with which this point is transported owing to the motion of the wave is called phase velocity. The phase velocity is given in terms of the wave’s angular frequency ω and wave vector k by,
vp = ω/k

15
Q

derivation of phase velocity

A

y = asin(ωt-kx)
k=2pi/lamda
When phase is constant, (wt – kx) = constant.
Differentiating, w - k d x /dt = 0
dx/dt = ω/k dx/dt = phase velocity, vphase = ω/k

16
Q

what is group waves

A

The group velocity of a wave is the velocity with which the variations in the shape of the
wave’s amplitude (known as the modulation or envelope of the wave) propagate through
space. The group velocity is defined by the equation, vg = dow/dok

17
Q

derivation of group waves

A

y1 = asin(wt+kx)
y2=asint[(w + deltaw)t- (k+deltak)x]
y= y1+y2
after manipulation
y = 2A cos {(Δω/2)t – (Δk/2) x} sin (ωt – kx)
Comparing equation 1 and 3, the amplitude is cosine term (2A cos {(Δω/2)t – (Δk/2) x} ),
which is not a constant but varies as a wave. The velocity with it is transmitted is group
velocity given by, vgr = dω/dk.

18
Q

what is HEISENBERG’S UNCERTAINITY PRINCIPLE

A

in Quantum Mechanics the moving particle is described by a wave packet. The particles should be inside wave packet, hence when wave packet is small; position of the particle may be fixed, but particle flies off rapidly
due to very high velocity; hence, its momentum cannot be determined
accurately. When the wave packet is large, velocity or momentum may be
determined but position of particle becomes uncertain.
According to uncertainty principle it is impossible to determine precisely and
simultaneously, the exact values of both members of particular pair of physical
variables which describes atomic system.
In any simultaneous determination of position and momentum of a particle, the
product of corresponding uncertainties inherently present in the measurements
is equal to or greater than h/4π.
Δp.Δx ≥h/4π
ΔE.Δt ≥ h/4π
ΔL.Δθ≥ h/4π

18
Q

what is Normalized functions

A

The value of ׀ψ׀2 evaluated at point gives the probability of finding a particle at that point, hence the probability of finding the particle inan element of volume δv is given by ψδv
Since the particle must be somewhere in space, the total probability of finding the particle should be equal to 1 i.e Any function which obeys this condition is said to be normalized Wave function

18
Q

The deBroglie waves are pilot waves and are not electro-magnetic waves.

A

bbsbsnsns

18
Q

Applications of Heisenberg’s Uncertainty Principle

A

 Non-existence of electrons in nucleus of atoms
 Calculation of frequency of radiation emitted by atom
 Calculation of binding energy of an electron in an atom
 Determination of radius of Bohr electronic orbit

19
Q

Physical significance of Heisenberg’s uncertainty principle

A

Non-existence of electrons inside the nucleus of atoms.
 Calculation of frequency of radiation emitted by an atom.
 Calculation of binding energy of an electron in an atom.
 Determination of radius of Bohr electronic orbit.
 The wave and particle properties are complimentary to one another.
 It is impossible to determine precisely and simultaneously values of
physical variables which describes the atomic system.
The negatively charged particle electron cannot exist inside the nucleus. The
wave and particle properties are complimentary to one another rather than
contradictory.

19
Q

what is a Wave Function

A

The concept of wave function was introduced by Schrödinger in the matter wave equation. It is denoted by Ψ, it is a variable whose variations constitutes matter wave. Wave Function is related to position of particle

19
Q

characteristics of wave function

A

1) The wave function by itself has no direct physical significance.
2) The wave function cannot be interpreted by an experiment.
3) The wave function is complex quantity consisting of both real and
imaginary parts.
4) With the knowledge of the wave function we can establish angular
momentum, energy and position of particle.
5) The value of │Ψ I^2evaluated at point gives the probability of finding particle at that point

19
Q

what is Probability Density?

A

The product of ψ and ψ* is ψψ* = a 2 + b2, which is called Probability density denoted by P = ׀ψ׀2

19
Q

properties of a wave function

A

Property 1: Ψ is single valued everywhere
Property 2:Ψ is finite everywhere
Property 3:Ψ and its first derivatives with respect to its variable are continuous everywhere.
Property 4: For bound states, Ψ must vanish at infinity. If Ψ is a complex function, then
ΨΨ* must vanish at infinity

19
Q

conditions of normalized waves functions

A

Normalized wave functions should satisfy following conditions:
1. It should be single valued function.
2. It should be finite everywhere.
3. It should be continuous and it should have continuous first derivative
ψ tends to zero when x, y, z tends to 0.

20
Q

what are Eigen’s values

A

Eigen functions are used in Schrödinger equation to solve for energy of a
system, since there can only be certain restricted Eigen functions and hence
only few restricted values of energy, these values of energy is called Eigen
values of energy.

21
Q

derivation of Schrödinger Time Independent Wave Equation

A

do doo nigha page 21

22
Q
A
22
Q
A
23
Q
A
23
Q
A
23
Q
A
23
Q
A
23
Q
A
23
Q
A
23
Q
A
23
Q
A
24
Q
A
24
Q
A
24
Q
A
24
Q
A
25
Q
A