Midterm 3 Flashcards

1
Q

Whichofthefollowingstatementsbestdescribesthequantumpropertyspin?
A)Spinisameasureoftherotationrateofasubatomicparticle
B)Spinisnotmeanttobetakenliterallybutmeasurestheinherentangularmomentumofasubatomicparticle.
C)Spinisapropertythatappliesonlytolargeobjects,likebaseballs.
D)Spinisameasureoftherateatwhichaparticlespinsaround(orbits)anotherparticle.
E)Spinisnotafundamentalpropertybutrathersomethingthatcanchangerandomlyatanytime.

A

Spinisnotmeanttobetakenliterallybutmeasurestheinherentangularmomentumofasubatomicparticle.

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2
Q

Anupquark(u)hasacharge+2/3,andadownquark(d)hasachargeof—1/3.Whichofthefollowingdescribesaproton?

A

uud

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3
Q

Thetwofamiliesof
fundamentalparticlesoutof
whichallordinarymattersmadeare

A

leptonsandquarks.

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4
Q

Thefourfundamentalforcesare

A

strongforce,weakforce,electromagneticforce,gravity

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5
Q
Supposethat,throughthemalicious
actofaneight-dimensionalalienbeing,
thestrongforcewassuddenlyturned
offthroughouttheuniverse.Whatwould
happenalmostimmediatelytoatoms?
A

Thenucleiofatomswouldfallapart.

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6
Q

Accordingtotheuncertaintyprinciple,

whichofthefollowingstatementsistrue?

A

Itisimpossibletomeasureboththeposition
andthevelocity ofaparticleatthe
sametime.

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7
Q
Whichofthefollowingstatementsbest
describestheexclusionprinciple?
A)Ifaparticlehasapreciselydefinedposition,
itisexcludedfromhavingapreciselydefined
momentum.
B)Twophotonscannotbeinthesameplace
atthesametime.
C)Thelawsofquantummechanicsare
excludedfromapplyingtolargeobjects
madeofmanyatoms.
D)Thelawsofquantummechanicsare
excludedfromourcommonsense.
E)Twofermionscannotoccupythesame
quantumstateatthesametime.
A

Twofermionscannotoccupythesame

quantumstateatthesametime.

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8
Q
Whichofthefollowingwillcause
thedegeneracypressurewithinanobject
toincrease?
A)compressingittohigherdensity
B)loweringitstemperature
C)lettingitexpandtolowerdensity
D)raisingitstemperature
E)shiningalightonit,whichaddsradiative
energy
A

compressingittohigherdensity

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9
Q

Whichofthefollowingstatementsabout
quantumtunnelingistrue?
A)Itisusedinmodernelectronics,and,
infact,ourmodern daycomputers
wouldnotworkwithoutit.
B)Itplaysacrucialroleinnuclearfusion
intheSun.
C)Itallowselectronsandothersubatomic
particlestopassthroughwall-likeenergy
barriersevenwhenitseemstheydo
nothaveenoughenergytogetthroughthebarriers.
D)Althoughithasbeenobservedtooccur,
itviolatesallotherknownlawsofnature,
andexplainingittherefore
representsamajorchallengetophysicists.
E)A,B,andCaretrue,butDisnot

A

E)A,B,andCaretrue,butDisnot

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10
Q

Whichofthefollowingbestexplains
thephenomenonofblackholeevaporation?
A)Blackholeevaporationisavirtualprocess,
meaningthatithasbeentheorizedbyastrophysicistsbutdoesn’treally
occur.
B)Particles(orantiparticles)arecreatedby
aquantummechanicaleffectnear,butoutside,
theeventhorizonoftheblack
hole.Thelawofconservationofenergymaintains
thattheblackholemustloseenergyto”pay”forthecreationofthis
mass.
C)Virtualparticlescreatedneartheblack
holeareconstantlyannihilatingeachother,causinga
veryhightemperature
eveniftheblackholehasnoaccretiondisk.
Thishightemperatureprovidesescapevelocityforthe
virtualparticles,causingtheentire”cloud”ofvirtualparticles
toexpandawayintospace.
D)Duetohightemperaturesintheaccretiondiskarounda
blackhole,materialevaporatesfromtheblackholelikewater
evaporatingfromtheocean.
E)Particles(orantiparticles)areoccasionallyejectedfrom
withintheeventhorizon,causingtheblackholetolosemass.

A

Particles(orantiparticles)arecreatedbya
quantummechanicaleffectnear,
butoutside,theeventhorizonofthe
blackhole.Thelawofconservationofenergy
maintainsthattheblackholemustloseenergyto
“pay”forthecreationofthis
mass.

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11
Q

Whichofthefollowingstatementsabout
degeneracypressureisnottrue?
A)Degeneracypressurestopsthegravitational
collapseofordinary(main­sequence)starsliketheSun.
B)Degeneracypressurearisesonlywith
fermions(suchaselectrons,protons,andneutrons)
andnotwithbosons(suchasphotonsorheliumnuclei).
C)Degeneracypressurestopsthegravitational
collapseofwhitedwarfs.
D)Explainingtheoriginofdegeneracy
pressurerequiresboththequantummechanicalexclusionprincipleandthe
uncertaintyprinciple.
E)Degeneracypressurehaltsthecollapse
ofneutronstars.

A

Degeneracypressurestopsthe

gravitationalcollapseofordinary(main­sequence)starsliketheSun.

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12
Q

Inthelate1800s,KelvinandHelmholtz
suggestedthattheSunstayedhot
thankstogravitationalcontraction.
Whatwasthemajordrawbackofthisidea?

A

ItpredictedthattheSuncouldlast
onlyabout25millionyears,whichis
farlessthantheageofEarth.

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13
Q

Whatdowemeanwhenwesaythat

theSunisingravitationalequilibrium?

A

ThereisabalancewithintheSun
between theoutwardpushofpressure
andtheinwardpullofgravity.

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14
Q

WhatistheSunmadeof?

A

70percenthydrogen,28percenthelium,

2percentotherelements

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15
Q

ThephaseofmatterintheSunis

A

plasma.

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16
Q

Fromthecenteroutward,whichofthe
followingliststhe”layers”oftheSun
inthecorrectorder?

A

core,radiationzone,convectionzone,

photosphere,chromosphere,corona

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17
Q

Sunspotsarecoolerthanthe

surroundingsolarsurfacebecause

A

strongmagneticfieldsslow
convectionandpreventhotplasma
fromenteringtheregion.

18
Q

Thefirststepintheproton­protonchainproducesananti­electron,orpositron.
Whathappenstothepositron?

A

Itisrapidlyconvertedtoenergywhen
itmeetsanordinaryelectron,resulting
inmatter­antimatterannihilation.

19
Q

Theoverallfusionreactionbywhich

theSuncurrentlyproducesenergyis

A

4H 1He+energy.

20
Q

Supposethat,forsomeunknownreason,
thecoreoftheSunsuddenlybecamehotter.
Whichofthefollowingbest
describeswhatwouldhappen?
A)Thehighertemperaturewouldnotaffect
thefusionratebutwouldcausethecoretoexpand
andcooluntilthetemperaturereturnedtonormal,
withthecoreatanew,slightlylargersize.
B)Highertemperaturewouldcausetherateof
nuclearfusiontorise,whichwouldincreasethe
internalpressure,causingthecoretoexpandand
turntheSunintoagiantstar.
C)Highertemperaturewouldcausetherateof
fusiontofall,decreasingtheinternalpressure
andcausingthecoreto
collapseuntiltherateoffusionreturnedtonormal.
D)Highertemperaturewouldcausetherateof
nuclearfusiontorise,whichwouldincreasethe
internalpressure,causing thecoretoexpandandcooluntilthe
fusionratereturnedtonormal.

A

Highertemperaturewouldcausetherateof
nuclearfusiontorise,whichwouldincrease
theinternalpressure,causing thecoretoexpandandcooluntilthe fusionratereturnedtonormal.

21
Q

Whathappenstoenergyintheconvectionzoneof

theSun?

A

Energyistransportedoutwardbytherising

ofhotplasmaandthesinkingofcoolerplasma.

22
Q

Whatprocessesareinvolvedinthesunspot

cycle?

A

thewindingofmagneticfieldlinesdueto

differentialrotation

23
Q

Sinceallstarsbegintheirliveswiththesame
basiccomposition,whatcharacteristicmost
determineshowtheywilldiffer?

A

masstheyareformedwith

24
Q

Astar’sluminosityisthe

A

totalamountoflightthatthestarwill

radiateoveritsentirelifetime.

25
Q

Ifthedistancebetweenusandastaris
doubled,witheverythingelseremainingthe
same,theluminosity

A

remainsthesame,buttheapparent

brightnessisdecreasedbyafactoroffour.

26
Q

Supposethatyoumeasuretheparallax
angleforaparticularstartobe0.5arcsecod.
Thedistancetothisstaris

A

2parsecs.

27
Q

Whichofthefollowingstatementsaboutspectral
typesofstarsistrue?
A)AstarwithspectraltypeAiscoolerthana
starwithspectraltypeB.
B)Thespectraltypeofastarcanbeusedto
determineitssurfacetemperature.
C)Thespectraltypeofastarcanbeusedto
determineitscolor.
D)AstarwithspectraltypeF2ishotterthana
starwithspectraltypeF3.
E)Alloftheabovearetrue.

A

Alloftheabovearetrue.

28
Q

Supposeyouseetwomain-sequencestars
ofthesamespectraltype.Star1isdimmerin
apparentbrightnessthanStar2byafactorof100.
Whatcanyouconclude?(Neglectanyeffectsthatmight
becausedbyinterstellardustandgas.)

A

Star1is10timesmoredistantthanStar2.

29
Q

Whichofthefollowingtermsisgiventoapairofstarsthatwecandetermineareorbitingeachotheronlyby
measuringtheirperiodicDopplershifts?
A)doublestar
B)spectroscopicbinary
C)visualbinary
D)eclipsingbinary
E)noneoftheabove

A

spectroscopicbinary

30
Q

OnaHertzsprung-Russelldiagram,wherewouldwefind

starsthathavethelargestradii?

A

upperright

31
Q

Youobserveastarinthediskofthe
MilkyWay,andyouwanttoplotthestaron
anH-Rdiagram.Youwillneedto
determineallofthefollowing,exceptthe

A

rotationrateofthestar

32
Q
Whichofthefollowingistrueaboutlow­massstarscomparedtohigh­massstars?
A)Low massstarsarehotterandmore
luminousthanhigh­massstars.
B)Low ­massstarsarecoolerandless
luminousthanhigh­massstars.
C)Low ­massstarsarecoolerbutmore
luminousthanhigh­massstars.
D)Low massstarshavethesametemperature
andluminosityashigh­massstars.
E)Low massstarsarehotterbutless
luminousthanhigh­massstars.
A

Low­massstarsarecoolerand

lessluminousthanhigh­massstars.

33
Q

WhyareCepheidvariablessoimportant

formeasuringdistancesinastronomy?

A

Theirluminositycanbe

inferredfromtheirperiod.

34
Q

Clusteragescanbedeterminedfrom

A

mainsequenceturnoff.

35
Q

Thetypicaldensityandtemperatureof

molecularcloudsare

A

300moleculespercubic

centimeter,10­30Kelvin.

36
Q

Ifyouwantedtoobservestarsbehind
amolecularcloud,inwhatwavelength
oflightwouldyoumostlikely
observe?

A

infrared

37
Q

Thethermalpressureofagasdepends

on

A

densityandtemperature.

38
Q

Whatpreventsthepressurefrom
increasingasacloudcontracts
duetoitsgravity?

A

Excesspressureisreleasedin

jetsofmaterialfromtheyoungstars.

39
Q

Whatisthelikelyreasonthat
wecannotfindanyexamples
ofthefirstgenerationstars?

A

Thefirstgenerationstarswere

allverymassiveandexplodedassupernova.

40
Q

Whendoesastar

becomeamain­sequencestar?

A

whentherateofhydrogenfusionwithinthestar’scoreis

highenoughtomaintaingravitationalequilibrium

41
Q

Whichofthefollowingdiscoveries,
iftheyexisted,wouldnecessitate
areevaluationofourideasofstellar
formation?

A

a0.01­

solar­massstar

42
Q

Whatpreventsabrowndwarf

fromundergoingnuclearfusion?

A

Degeneracypressurehaltsthecontraction
ofaprotostarsothecoreneverbecomes
hotordenseenoughfornuclearfusion.