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Page ‹#› AS 4022 Cosmology Lecture 4 Space-Time Metric AS 4022 Cosmology Olber’s Paradox Flux from all stars in the sky : F = n F d Vol ( ) = n L A( χ ) A χ ( ) Rdχ ( ) 0 χ max = n L R χ max ⇒∞ for flat space, R →∞. A dark sky may imply : (1) an edge (we don't observe one) (2) a curved space (finite size) (3) expansion (R(t ) => finite age, redshift ) Why is the sky dark at night ? AS 4022 Cosmology Minkowski Spacetime Metric ds 2 = c 2 dt 2 + dl 2 dτ 2 = dt 2 dl 2 c 2 = dt 2 1 1 c 2 dl dt 2 Null intervals light cone: v = c, ds 2 = 0 Time-like intervals: ds 2 < 0, dτ 2 > 0 Inside light cone. Causally connected. Space-like intervals: ds 2 > 0 , dτ 2 < 0 Outside light cone. Causally disconnected. dτ = -ds 2 / c 2 =dt 1- v 2 c 2 > 0 Photons arrive from our past light cone. World line of massive particle at rest. Proper time (moving clock): AS 4022 Cosmology Minkowski Spacetime Metric ds 2 = c 2 dt 2 + dl 2 dτ 2 = dt 2 dl 2 c 2 = dt 2 1 1 c 2 dl dt 2 Null intervals light cone: v = c, ds 2 = 0 Time-like intervals: ds 2 < 0, dτ 2 > 0 Inside light cone. Causally connected. Space-like intervals: ds 2 > 0 , dτ 2 < 0 Outside light cone. Causally disconnected. dτ = -ds 2 / c 2 =dt 1- v 2 c 2 > 0 Photons arrive from our past light cone. World line of massive particle in motion. Proper time (moving clock): AS 4022 Cosmology Robertson-Walker metric uniformly curved, evolving spacetime ds 2 = c 2 dt 2 + R 2 (t ) dχ 2 + S k 2 χ ( ) dψ 2 ( ) = c 2 dt 2 + R 2 (t ) du 2 1 ku 2 + u 2 dψ 2 = c 2 dt 2 + a 2 (t ) dr 2 1 krR 0 ( ) 2 + r 2 dψ 2 dψ 2 dθ 2 + sin 2 θ dφ 2 a(t ) R(t )/ R 0 R 0 R( t 0 ) S k (χ) = sin χ (k =+1) closed χ (k = 0) flat sinh χ (k = 1) open D R χ w r radial distance = D(t ) = R( t ) χ circumference = 2 π r(t ) r(t ) = a(t ) r = R(t ) u = R( t ) S k χ ( ) AS 4022 Cosmology Redshift and Time Dilation Light rays are null geodessics : ds 2 = R 2 ( t ) dχ 2 c 2 dt 2 = 0 dχ = c dt R( t ) χ = c dt R(t ) + e t e t + e Δt c dt R( t ) e t + e Δt o t = c dt R( t ) + e t + e Δt o t c dt R(t ) o t o t + o Δt Δt e R( t e ) = Δt o R( t o ) R(t o ) R(t e ) = Δt o Δt e = λ o λ e = 1 + z Observed wavelengths and time intervals appear "stretched" by a factor x = 1 + z = R 0 R( t ) . χ t t 0 + Δt 0 t e t 0 t e + Δt e

Transcript of Page - University of St Andrewsstar-kdh1/cos/cos04c.pdfPage ‹#› AS 4022 Cosmology Lecture 4...

Page 1: Page - University of St Andrewsstar-kdh1/cos/cos04c.pdfPage ‹#› AS 4022 Cosmology Lecture 4 Space-Time Metric AS 4022 Olber’s Paradox € Flux from all stars in the sky: F=∫n

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AS 4022 Cosmology

Lecture 4

Space-Time Metric

AS 4022 Cosmology

Olber’s Paradox

Flux from all stars in the sky :

F = n∗ F∗ d Vol( )∫ = n∗L∗A(χ)

A χ( ) R dχ( )

0

χmax

= n∗ L∗ R χmax

⇒∞ for flat space, R→∞. A dark sky may imply : (1) an edge (we don't observe one) (2) a curved space (finite size) (3) expansion (R(t) => finite age, redshift )

Why is the sky dark at night ?

AS 4022 Cosmology

Minkowski Spacetime Metric

ds2 = −c 2dt 2 + dl2

dτ 2 = dt 2 − dl2

c 2= dt 2 1− 1

c 2dldt

2

Null intervalslight cone:v = c, ds2 = 0

Time-like intervals:ds2 < 0, dτ2 > 0

Inside light cone.Causally connected.

Space-like intervals:ds2 > 0 , dτ2 < 0

Outside light cone.Causally disconnected.

dτ = -ds2 /c 2

= dt 1- v2

c 2> 0

Photons arrivefrom our pastlight cone.

World lineof massiveparticleat rest.

Proper time (moving clock):

AS 4022 Cosmology

Minkowski Spacetime Metric

ds2 = −c 2dt 2 + dl2

dτ 2 = dt 2 − dl2

c 2= dt 2 1− 1

c 2dldt

2

Null intervalslight cone:v = c, ds2 = 0

Time-like intervals:ds2 < 0, dτ2 > 0

Inside light cone.Causally connected.

Space-like intervals:ds2 > 0 , dτ2 < 0

Outside light cone.Causally disconnected.

dτ = -ds2 /c 2

= dt 1- v2

c 2> 0

Photons arrivefrom our pastlight cone.

World lineof massiveparticlein motion.

Proper time (moving clock):

AS 4022 Cosmology

Robertson-Walker metricuniformly curved, evolving spacetime

ds2 = −c 2dt 2 + R2(t) dχ 2 + Sk2 χ( ) dψ 2( )

= −c 2dt 2 + R2(t) du2

1− k u2 + u2 dψ 2

= −c 2dt 2 + a2(t) dr2

1− k r R0( )2 + r2 dψ 2

dψ 2 ≡ dθ 2 + sin2θ dφ 2

a(t) ≡ R(t) /R0

R0 ≡ R(t0)

Sk (χ) =

sinχ (k = +1) closedχ (k = 0) flat

sinhχ (k = −1) open

DR

χ w

r

radial distance = D(t) = R(t)χ circumference = 2π r(t) r(t) = a(t) r = R(t) u = R(t)Sk χ( )

AS 4022 Cosmology

Redshift and Time Dilation

Light rays are null geodessics :ds2 = R2(t) dχ 2 − c 2 dt 2 = 0

dχ =c dtR(t)

χ =c dtR(t)

+et

et +eΔt

∫ c dtR(t)

et + eΔt

ot∫ =

c dtR(t)

+et + eΔt

ot∫ c dt

R(t)ot

ot +oΔt

ΔteR(te )

=ΔtoR(to)

→ R(to)R(te )

=ΔtoΔte

=λoλe

=1+ z

∴Observed wavelengths and time intervals appear "stretched" by a factor x =1+ z = R0 R(t).

χ

t

t0 + Δt0

te

t0

te + Δte

Page 2: Page - University of St Andrewsstar-kdh1/cos/cos04c.pdfPage ‹#› AS 4022 Cosmology Lecture 4 Space-Time Metric AS 4022 Olber’s Paradox € Flux from all stars in the sky: F=∫n

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AS 4022 Cosmology

Fidos and co-moving coordinates

Distance varies intime:

D(t) = R(t) χ

“Co-moving” coordinates

χ or D0 ≡ R0 χ

D(t)

t

Dt

χ

“Fiducial observers”(Fidos)

Labels the Fidos

AS 4022 Cosmology

Cosmological Principle

All “co-moving”observers see anequivalent view.

Light ray

Past light cone:

- looking out = back in time

AS 4022 Cosmology

Coordinate Systems

AS 4022 Cosmology

Conformal time

t

χ

η ≡c dtR( t)∫

Stretch time axis to make light rays at 45o.

χ

η

ds2 = R2(t) −dη2 + dχ 2 + Sk2(χ)dψ 2( )

AS 4022 Cosmology

The Horizon: How far can we see?

• We see only a finite patch of the Universe.

• The Horizon may grow with time (if expansiondecelerates) or shrink in time (e.g. inflation).

suppose R(t) = R0 t t0( )α

χH =η0 =c dtR(t)0

0t∫ =

c t01−α( ) R0

if α <1

⇒ ∞ as α ⇒1 1/2

:dominated-radiation

2/3

: dominated-matter

=

=

α

α

η0

χH

−χH

0AS 4022 Cosmology

Angular Diameter Distance

• radial distance– now ( when photon received ):

– when photon emitted:

• angular size– Fraction of circumference when photon was emitted:

• angular diameter distance

D0 = R(t0) χ = R0 χ

DA ≡lθ

= r(te ) = R(te ) Sk (χ) =R(te )R0

R0 Sk (χ)

=R0 Sk (χ)

1+ z=r(t0)1+ z

≡r0

1+ z

χ0

te

to

D0

De

De = R(te ) χ =R(te ) R0 χ

R0=D0

1+ z

θ2π

=l

2π r(te )

l

θ

Circumference wassmaller by factor x=1+z.

Souces look larger/closer.

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AS 4022 Cosmology

Luminosity Distance

– Luminosity ( erg s-1 )

– area of photon sphere ( when photons observed ):

– redshift:

– time dilation: lower photon arrival rate

– observed flux ( erg cm-2 s-1 )

• Luminosity distance

F =N h ν 0A0 Δt0

=L

4π r02 1+ z( )2

=L

4π DL2

DL = 1+ z( ) r0 = (1+ z)R0 Sk (χ)

A0 = 4π r02 = 4π R0

2Sk2(χ)

λ0 = λe (1+ z)ν 0 = ν e 1+ z( )

L =N h νeΔte

Δt0 = Δte (1+ z)

χ0

te€

t0

Δte€

Δt0

Sources lookfainter/farther.

AS 4022 Cosmology

Surface Brightness

• Solid angle

• Surface brightness– Flux per solid angle (erg s-1 cm-2 arcsec-2)

– decreases very rapidly with z because:

– expansion spreads out the photons

– decreases their energy

– decreases their arrival rate€

Σ≡FΩ

=L

4π DL2DA

2

A=

L4π A 1+ z( )4

ADA

DA A2/=Ω

DL = 1+ z( ) r0

DA =r0

(1+ z)r0 = R0 Sk (χ)

AS 4022 Cosmology

Flux Density Spectra• emitted photons

– (erg s-1 Hz-1)

• redshift photon numbers

• observed flux density spectra– (erg cm-2 s-1 Hz-1)

– (erg cm-2 s-1 A-1)

Fν λo( ) =N λo( ) h ν 0Δν 0 Δt0 A

=Lν λe( )4π DA

21

(1+ z)

Fλ λo( ) =N λo( ) h ν 0Δλ0 Δt0 A

=Lλ λe( )4π DA

21

(1+ z)3

Lν λe( ) =N(λe ) h νeΔνe Δte

λo = λe(1+ z )

N λo( ) = N λe( )