Mean Free Path - Physics - Past Exam, Exams of Physics

This is the Past Exam of Physics which includes Kepler Third Law, Total Lunar Eclipses, Ecliptic, Types of Electromagnetic Radiation, Astronomical Telescopes, Constellations of Zodiac, Twin Paradox, Fundamental Forces etc. Key important points are: Mean Free Path, Kinetic Temperature, Steady State, Thermal Conductivity, Constant Pressure, Change in Entropy of Gas, Optical Spectrum, Refractve Index, State of Polarisation

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2012/2013

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NATIONAL
UNIVERSITY
OF SINGAPORE
PC1142
Physics
ll
(Semester
l:
AY 2009-10,
28 November
2009)
Time Allowed:2
Hours
INSTRUCTIONS
TO CANDIDATES
1. This
examination
paper
comprises EIGHT
(8)
printed
pages
with FIVE
(5)
short
questions
in
Part
'l
and
THREE
(3)
long
questions
in
Part 2.
2. Answer ALL
questions.
3. The total marks
for Part 1 is 40
and for Part 2 is
60.
4. Answers
to the
questions
are
to be written in
the answer
booklet
provided.
5, This is a CLOSED
BOOK
examination.
Calculators are
allowed.
6. A list
of
physical
constants and formulae
is
given
on
pages
2
and 3,
pf3
pf4
pf5
pf8

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NATIONALUNIVERSITYOFSINGAPORE

PC1142Physics

ll

(Semester l: AY2009-10, 28November2009)

TimeAllowed:2Hours

INSTRUCTIONS

TOCANDIDATES

  1. Thisexaminationpaper comprisesEIGHT

(8)printedpages withFIVE(5)shortquestions in

Part

'l

andTHREE(3)longquestionsinPart2.

  1. AnswerALL

questions.

  1. ThetotalmarksforPart 1 is40andforPart 2 is60.
  2. Answerstothe

questions are tobewrittenintheanswerbooklet

provided.

5, Thisisa CLOSEDBOOKexamination. Calculatorsareallowed.

A list ofphysicalconstantsandformulaeisgivenonpages 2 and3,

Thermal

physics andkinetictheory:

(i) Kinetic mean free path is

given by

4

I = --: - , where

nvis thenumber density

J Z x. n , ' d 2

andd isthemolecular diameter.

(ii) Maxwell-Boltzmanndistributionin3D:

/ l 3 l 2 r a

P(v)

= 4n.n'-(

l"''.

,rJ-

t '

u'

\ 2 n. k ,. r)

' \ _ r u , - ,

(a)Root-mean-squarespeed:

y-^ = ^ltrt' .

V m

(v).Oneform of adiabat:p .Vv = Constanf .

(vi)Stefan-Boltzmann equation: P,"a

= 6. A.e .Ta

(vii)Planck radiationequation:

2 n. h. c 2

f o a l r , ) = m

r'.[*o[

^

n,''

=l-rl

[

(. r' k , ' T

(viii)Wiendisplacement law:

" 2.898x10-3m

.K

lu

peak

=

(ix) Convectionequation: Pror,

= h. A. LT.

(x)Conductionequation:

Pcond

= -k A +

L

(xi)Linear thermalexpansion: AL= cr.L.LT.

(b)Averagespeed:

v,,

(c)Most-probable speed: ,," =

^l2krT '

l l m

(iii) ldealgasequation:p .V = n .R.T .

(iv) VanderWaalsequation:

^ ^ 2

( p +

o ' l '

). ( v- n. b )

= n ' R. T.

" v z

Thermodynamics:

(i)First lawof thermodynamics:LU

= qin

  • Win.Gas

expansionworkdonebythegas: W,,,

=

[p

.dV.

(ii)Carnotheat-engine efficiency e. =1-L.

" T ,

Geometricoptics:

(i)p and

q are objectandimage distancesmeasured

respectivelyon oppositesidesof thelensor of the

refracting surface:

(a) Object-imagerelation(thin

wherel=(n-1)

ff

-f)

t

' . R ,

R r )

(b)Refracting-surfaceequation:

bns):

1*

1

=

1

,

p q t

f r t

,

D z

_ f l 2 - D t

p q R

(iii)Enhopy

dS

=

dg',n

.

T

(iv)EnthalpyH= E+ PV.

(v)HelmholtzfreeenergyF = E- IS.

(vi)Gibbs freeenergyG

= H- IS,

(ii) Gullstrand equation:

(a)Effectivepower:

P = P, +

p,

(b)Fronfvertexrefractingpower:

P. -P. +

P

. t. ,

n

p r. d

n

(c)Back-vertex refractingpower:

P. - P *

q

. o. ,

n

q. d

n

  • P ' P r '!

' - n

SkBT

nn

PC1142Physicsll

Part1 Answer allFIVE

questions. Allquestionscarry 8 markseach.

  1. Thedarknebulaininterstellarspaceisthought tocontain50hydrogen(H)atomspercubic

centimetre.Thesehavea root-mean-squareSpeedof 1400 m s-1.

[Nofe:

H hasan

atomicweightof1,

g mol-t anda diameterof1.0A.l

(i) Compute themeanfree

path oftheseHatoms,

(ii) Compute theirkinetictemperature.

  1. Considera blackbodyinvacuumcomprisinga thermally-conductive solidcoreofradiusrc

andhavinga uniformtemperatureI', surroundedbya thermally-insulating solid shell

of

thicknessd withthermalconductivityk,asshownbelow.Heat isproducedinternallyinthe

coreata rateof P. Derive anexpressionforthevalueof I, atsteady state,intermsofP,

k,16,d,andothernecessaryconstants.

vacuum

1,0kgof helium

gasis heatedatconstant

pressure

from 300 K to600K. Computethe

changeinentropy ofthe

gas.[Nofe: Hehasanatomicweightof4.0g moFt,]

  1. A camerawith aneffectivefocallength of 300 mmandF-number of 5.6is used torecord

theopticalimageof theground fromanaeroplane flying10kmaboveground. Canthis

cameraresolvea carontheground, if thelens systemis freefrom aberrations,basedon

Rayleigh'scriteria?

[Nofe:

The opticalspectrumspans 450-650nm.]

  1. Waveplates are opticalelements designedto differentially retardthe phase of the

components of a polarisedbeam.One suchwave

plate ismade ofbirefringent crystalline

quartz withanordinary refractiveindex(no) of 1.5426andanextraordinary refractive index

(ne) of 1.5517at a wavelength of632.8nm,and orientedasshown below.Thefast axis

hastheindex no,whiletheslow axishasindexnr, The thicknessof theplateis 1.00g

mm.

A linearlypolarised beamof 632.8-nm lightis incident normallywiththe plane of

polarisation

at anangle0 measured clockwisefromthefastaxis.Compute thephase shift

between lhecomponent

polarised parallel tothefastaxis andthat

polarised parallel tothe

slowaxis,andgive thestateofpolarisation after

passing thiswaveplate.

  1. Achromaticdoubletlenseshave significantlybetteropticalperformance thansinglet lenses

for imagingapplications.An achromat(general structureshown below)consistsof a

positivelow-index crown

Elass

lenselementwithradii of curvature h ?ndh, andcentre

thickness fcr,ceffiertodto a negativehigh-indexflintglass lenselementwithradil of

curvature h and

rl, ?fldcentre thicknessfcz.Theselens elementsarechosen so asto

cancel chromaticabenationat the red (630-nmwavelength) and blue(450nm)

wavelengths.Onesuchachromat hasa diameterof 6.35mmandis constructedwithrr

8.609mm,rz=-5,134mm,ta = 2.7mm, andtcz

0] mm. lt hasaneffective focallength

(EFL)

of 12.7mmat 589-nmwavelength.Therefractive indexforthecrownglass usedis

1,52andforflint

glass is 1.66at thiswavelength. BFL

= back

focallength, FFL

= front

focallength.

(i) Compute thevalueofrr inthethin-lens

paraxial ray approximation.

[8marks]

(ii) Compute thelateralmagnificationoftheimage ofanobjectlocated12, minfront

ofthelens,

(iii) Brieflyexplainthemeaningof

"chromatic

aberration"

[8marks]

[4marks]

  1. Whentwoor morewavesarepresentinthesameregion of space,theresultantwaveisa

superposition oftheindividualwaves.

(i) Considerthesuperposition of twomonochromaticcoherent

plane waves with

amplitudes0r ?fldazrospectively, and

phases

0r

and

$zrespectively,

Showthat

theintensityoftheresultantwaveisgivenby:

I = 11+t2 +2r[tfucosA, where 4 =

Q

  • gr.

[Bmarks]

Considernowthatthesetwowaveshave equalintensities/0,buttheytravelatan

anglewitheachother.Onewavetravelsalong the+z-direction,whiletheother

wavetravels at anangle0 withthez-axisin thexzplane,asshown below.Atthe

overlaponthexyplane,a sinusoidal

pattern ofbright anddarkfringesisformed.

(a) Show thatthephasedifferencebetweenthetwowaves measuredalongx

varies accordingto A = x4sing

t8marksl

(b) Fromthe resultof (i) aboveor othenruise,derive the equationthat

describestheintensityvariation inthex-directionofthisinterferencepattern.

[4marks]

- END

OFPAPER

(ii)

PH