Lecture Mod Phys Fall 2014 NPG 2 Black Body

15
BLACK BODY RADIATION BLACK BODY RADIATION 1

Transcript of Lecture Mod Phys Fall 2014 NPG 2 Black Body

Page 1: Lecture Mod Phys Fall 2014 NPG 2 Black Body

BLACK BODY RADIATIONBLACK  BODY RADIATION

1

Page 2: Lecture Mod Phys Fall 2014 NPG 2 Black Body

Black Body RadiationBlack Body Radiation

Black Body :‐ It absorbs all radiation it receivesBlack Body : It absorbs all radiation it receives

Practical Realization A I th l it ith ll t th hPractical Realization:  An Isothermal cavity with a small aperture through which radiation from out side can be admitted

ρ(υ) dν = energy per unit volume of cavity is contributedρ(υ) dν energy per unit volume of cavity is contributed by the radiation between ν and ν + d ν

2

Page 3: Lecture Mod Phys Fall 2014 NPG 2 Black Body

Black Body RadiationBlack Body Radiation

Black Body :‐ It absorbs all radiation it receivesBlack Body : It absorbs all radiation it receives

Practical Realization A I th l it ith ll t th hPractical Realization:  An Isothermal cavity with a small aperture through which radiation from out side can be admitted

ρ(υ) dν = energy per unit volume of cavity is contributed by the radiation between ν and ν + d ν

3

Page 4: Lecture Mod Phys Fall 2014 NPG 2 Black Body

Blackbody Radiation Spectrum

Energy densityin the windowυ and υ +d υ

ρ(υ)T=1400 K

T=1800 Kρ(υ)J/m -Hz3

T=1000 K

frequency υ4

Page 5: Lecture Mod Phys Fall 2014 NPG 2 Black Body

Lord Rayleigh- James Jeans LawLord Rayleigh James Jeans LawNumber of independent standing waves in the frequency interval  

G (υ) dυ =  8πυ2 dυ / c3According to the theorem of equipartition 

L = 2(λ/2)g q p

energy , the average energy per degrees of freedom = ½ kT.  Each standing wave originates from oscillating electric charge  in the wall and  2 degrees of freedom is associated ith the

ε = kT2 degrees of freedom  is  associated with the wave . Hence average energy   L =λ/2

ε kT

5

Page 6: Lecture Mod Phys Fall 2014 NPG 2 Black Body

Ultrasonic Catastrophe

T=1800 K

( )T=1800 K

ρ(υ)

T=1400 KT=1000 K

frequency υ6

Page 7: Lecture Mod Phys Fall 2014 NPG 2 Black Body

ρ(υ) T=1800 K

υ dependence2

frequency υ7

Page 8: Lecture Mod Phys Fall 2014 NPG 2 Black Body

Planck’s Formula

when hυ << kT

Rayleigh Jeans law

when  hυ << kT

Rayleigh-Jeans law

when  hυ >> kTυ large

8Wien’s law ρ(v) dv = (8πv2/c3 )(hv)e-hv/kT dv

Page 9: Lecture Mod Phys Fall 2014 NPG 2 Black Body

Planck’s Concept of Energy Quantization

14th December, 1900

νhE = νhE =

Max Karl Ernst Ludwig Planck1858‐1947 9

Page 10: Lecture Mod Phys Fall 2014 NPG 2 Black Body

Planck’s postulateAny physical entity whose ``co-ordinate” is oscillating sinusoidally with frequency y can possess only total energies E as integral multiple of

h = Planck’s constant

42Classical

E = 0 10

Page 11: Lecture Mod Phys Fall 2014 NPG 2 Black Body

εn = nhv, n = 0, 1, 2, 3,….r

No. of oscillators with energy εn is proportional to e-εn/ kT

. If there are N oscillators and E be the total energy, the average energy ε = E/N. Let there be No , N1 , N2 ,…Nr

ill h i 0 h 2h h d N Noscillators having energy 0, hv, 2hv ,…,rhv and Nr = No e-rhv/ kT

N = N + N + N + +NN = No + N1 + N2 + … +NrE= 0. No e-0/ kT + No hv. e-hv/ kT +No 2hv.e-2hv/ kT +………+

N rhv e-rhv/ kTNo rhv.e

11

Page 12: Lecture Mod Phys Fall 2014 NPG 2 Black Body

N = No (e-0/ kT + e -hv/ kT + e -2hv/ kT +………+ e -rhv/ kT )= N / ( 1- e-hv/ kT ) [ 1+x + x2 + x3 + …= 1 /(1-x) ] No / ( 1 e ) [ 1+x + x + x + … 1 /(1 x) ]

E = No hv. e-hv/ kT (1+ 2e-2hv/ kT +………+ re -(r-1)hv/ kT )

= No hv. e-hv/ kT {1/ (1- e-hv/ kT ) }2 [ 1 + 2x + 3 x2 +.. = 1/(1-x)2 ]

ε = E/N

ε = 

12

Page 13: Lecture Mod Phys Fall 2014 NPG 2 Black Body

Planck’s FormulaPlanck s Formula

13

Page 14: Lecture Mod Phys Fall 2014 NPG 2 Black Body

Wien’s displacement Law

Wien's displacement law states that the wavelength distribution of thermal radiation from a black body at any temperature has essentially the same shape as the distribution at any other temperature except that each wavelength isas the distribution at any other temperature, except that each wavelength is displaced on the graph.

14

Page 15: Lecture Mod Phys Fall 2014 NPG 2 Black Body

15