Top Banner
Connoting Rm=Oc3 . In - oil [ %I%]f . . . - - - . ! conformal Hubble team , COOO , Apc i k LH a super - horizon / horizon todas i ( Ya > you i 109pct - - - - - - - d today ao= I c y - today in ¥2 : dpns - a. doom ' Mpe - n - - I - - . ' dphy today ) = doom ( today ) I , I ' , Iya # ! uguggpigaeaodg npaqsic.ae , aan . 1 Human rig ( Tumey , i microscopic sale at ( micro - 3mm I ' Abeg.hr i scopfc . . lsec-y-F.IT time ( Ne - 40 , begin inflation end RDE rude 1nA Two "Gev - ardBigBaug, cosmo for general public standard cosmology for scientists te = Be longer = Ae co - 514ps = Indeed a begin F- offer - Kisa Ne - Stege = few Ot - NHI = Ne - lo -" see ~ co - Hse ,
7

conformal Hubble 109pctjyoo/class/2020/notes4.pdfI = in-ton point mass → mass distribution → fluctuation → Snc on over distance test potentialfluctuation point mass of ie Esta

Mar 06, 2021

Download

Documents

dariahiddleston
Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Page 1: conformal Hubble 109pctjyoo/class/2020/notes4.pdfI = in-ton point mass → mass distribution → fluctuation → Snc on over distance test potentialfluctuation point mass of ie Esta

Connoting Rm=Oc3 . In - oil

[%I%]f. . . .

-- - - .

. ! conformal Hubble team, COOO

, Apc i k LH a super - horizon/

horizon todasi ( Ya > you

i 109pct- - - - - - - - d today ao= Ic y-

today in ¥2: dpns - a. doom' Mpe - n - - - -

I- -

-- .

' dphy today ) = doom (today )I ,

I

'

,Iya# ! uguggpigaeaodg → npaqsic.ae, aan.

1 Human rig ( Tumey ,i

→ microscopic sale at( micro -

3mm I ' Abeg.hri scopfc

..lsec-y-F.IT time (Ne- 40,

③ begin inflation end RDE rude 1nATwo"Gev-

ardBigBaug, cosmo for general publicstandard cosmology for scientists

te = Be longer = Ae co-514ps =

Indeedabegin

F- offer - Kisa Ne- Stege = fewOt - NHI = Ne - lo

-"see ~ co

-Hse,

Page 2: conformal Hubble 109pctjyoo/class/2020/notes4.pdfI = in-ton point mass → mass distribution → fluctuation → Snc on over distance test potentialfluctuation point mass of ie Esta

Ds-

weak gravitational lensing M-

%7F¥/strong . weak . Miao tensing

.jp/sb!,-↳ snc

- → ZEN real-Ok = ¥% n d = ÷M÷ . as b.a ' a position

* relativistic connection : sector 2.

a - IET $8919771Ds . I = Ds ' b - Dhs - a

£ = in - Apes a = in - Ott lens equation

r2

= Dis 4914b = Die ' n AE -

-

DsDh C-

point mass I - ri - GEINEinstein readies Qe =

→ arcsecftf.dk/FzJdk/i-tf;eJ"

Page 3: conformal Hubble 109pctjyoo/class/2020/notes4.pdfI = in-ton point mass → mass distribution → fluctuation → Snc on over distance test potentialfluctuation point mass of ie Esta

I = in - ton point mass → mass distribution → fluctuation → Snc

on over distance test '

potential fluctuation

point mass of ie Esta.

a- 45¥

I = in - GOI.BE = oh

.E : projected leasing potential

* mass distribution : OI = Is t¥ SAZ - 24 cylindrical coordinate-

D't = 44958 .62£ = 4¥ Azz SS = 2¥ .

E - Sdh' Ezln in -ng← lensing kernel

* fluctuation over distance i § - Eden ( 24 = Sabr . Serj' ay• e gere . =

h '

-

w e e

rg←angular diameter distance

* src distribution e § - Goodine B) 2X.

g= r://drst.br/nscrsl in firing ers ,-

Page 4: conformal Hubble 109pctjyoo/class/2020/notes4.pdfI = in-ton point mass → mass distribution → fluctuation → Snc on over distance test potentialfluctuation point mass of ie Esta

robot§ - ri - ohh i position . geodesic

dose - ten - ton : shape . geodesic deviation

dsi - Disdain . Dis - IFT -- Tsi; - ( III. ¥: ) - I - (Ko : ) - ( E .'t. ) - Gow ow )

K - e- Ier = IC# e- Ear).

w= I c - Dal = - ICE, - OIL)YE ICD

se- Dal - ICE. - Ess ) .

Tse - I kDa) = OI , , -82 ,

Eiji I. DIE = stregcrs.rs Diffdef '- cc-42- V'+ w

'

re c - 2K

②2 Snc

. wordn n

a.EE"

figs,

m - III. - aan→ A

= It 2K

g Xx

x

dA= 0×8, DSi - Dli , Q, dAsrc=DiiDis0xOyObs

8SF=lDizDg =detDidAobs

Page 5: conformal Hubble 109pctjyoo/class/2020/notes4.pdfI = in-ton point mass → mass distribution → fluctuation → Snc on over distance test potentialfluctuation point mass of ie Esta

Obs lensSrc

TEH # s-

a

galaxyObs. galaxychip-

ellipticity EE dib I f t dat G - at i - g

fMtb

×

E-cee.exi-lmmIIYIT.ae?IIImI=ecwsaop.sina@Idsi--Diddy → dhi=dDYigdsg

Obs

Mignon Warming ~ St's ID'll Wcs) (Digits ( Beltoise~ idol )jelD4 Mice

eiibs = et't so, c- Out D'- ¥, (

' ' II" I:* )@Ibs = EEN t 28, + OCH

Page 6: conformal Hubble 109pctjyoo/class/2020/notes4.pdfI = in-ton point mass → mass distribution → fluctuation → Snc on over distance test potentialfluctuation point mass of ie Esta

E:b = desk-121, no lensing G- = EAS2B E - o - I

Exons = Exsrc ← 28, K - 82=0 Eq = @ sing D= o - 1800

Ipt{ Et> ~ NI? Etcxi ) ~ LEKAS S - o = ( Ex>@e- Ex> = ICE> oink@> →[Lee> aced > = Leastwise > = Ile's

apt ( Etch ) Ee Cui > ,Lex & )

.Let

↳ = .ee?IE'Se4oe.ki.stfei*staetsFa#y ~ coat-5

.Esr - 0.3 188$33,u. -33

to

Page 7: conformal Hubble 109pctjyoo/class/2020/notes4.pdfI = in-ton point mass → mass distribution → fluctuation → Snc on over distance test potentialfluctuation point mass of ie Esta

(EI? exo" ) → CA . 8×1 n 8%03 in) →

[email protected] Bon

% .

"¥'