Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t...

21
Introduction to Cosmology Lecture 5

Transcript of Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t...

Page 1: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z

Introduction to CosmologyLecture 5

Page 2: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 3: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 4: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 5: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 6: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 7: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 8: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z

0 0(t +dt , 0)

1 1 1(t +dt , r )

lineP’s world

lineO’s world

(t , 0)0

1 1(t , r )

Page 9: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 10: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 11: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 12: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z

Ωm,0 = 0.3, ΩΛ,0 = 0.7

Ωm,0 = 0.3, Ωk,0 = 0.7

Ωm,0 = 0.0, Ωk,0 = 1

Page 13: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 14: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 15: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z

Ωm,0 = 0.3, ΩΛ,0 = 0.7

Ωm,0 = 0.3, Ωk,0 = 0.7

Ωm,0 = 0.0, Ωk,0 = 1

Page 16: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 17: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 18: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 19: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 20: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z
Page 21: Introduction to Cosmology Lecture 5pettini/Intro... · Introduction to Cosmology Lecture 5. 0 0 (t +dt , 0) (t +dt , r ) 1 1 1 line P’s world line ... —0.3 open . 9 Redshift z

Angular size of typical CMB patch


Magnetic inductance Solenoids - Universitetet i oslofolk.uio.no/ravi/cutn/elec_mag/16_maxwell_difform.pdfBdA 0 G’L f Mi A BdA 0 Gauss’s aw or Magnetism B CA dd Ed BdA dt dt Faraday’s

Magnetic inductance Solenoids - Universitetet i oslofolk.uio.no/ravi/cutn/elec_mag/16_maxwell_difform.pdfBdA 0 G’L f Mi A BdA 0 Gauss’s aw or Magnetism B CA dd Ed BdA dt dt Faraday’s

MASSIVE NEUTRINOS AND COSMOLOGY

MASSIVE NEUTRINOS AND COSMOLOGY

Scalar Field Cosmology - kpfu.ru

Scalar Field Cosmology - kpfu.ru

DT.VAG-PTD1 - FACOM FRANCE | - Accueil · dt.4444 dt.3054v3 dt.4633 dt.4635 dt .4451 dt.4115a-1 d . 47 9 dt.4401 dt.5000 dt.4809 dt.4440t1 dt.5008 dt.4440v2 dt.4440v1 vag oem facom

DT.VAG-PTD1 - FACOM FRANCE | - Accueil · dt.4444 dt.3054v3 dt.4633 dt.4635 dt .4451 dt.4115a-1 d . 47 9 dt.4401 dt.5000 dt.4809 dt.4440t1 dt.5008 dt.4440v2 dt.4440v1 vag oem facom

21cm cosmology

21cm cosmology

On cosmology, infinities, and zeta functions

On cosmology, infinities, and zeta functions

Age Crisis (~1995) HLecture 9 Observational Cosmology ...

Age Crisis (~1995) HLecture 9 Observational Cosmology ...

The KEK-All Ion Accelerator (KEK-AIA) · 2π/ω Acceleration region dB/dt Acceleration voltage requirement always transient from 0 V to peak to 0 V Solution - Pulse density control

The KEK-All Ion Accelerator (KEK-AIA) · 2π/ω Acceleration region dB/dt Acceleration voltage requirement always transient from 0 V to peak to 0 V Solution - Pulse density control

issue-42.Dt 02.07.12-08.07.12

issue-42.Dt 02.07.12-08.07.12

Penyakit Jantung Rematik Dt

Penyakit Jantung Rematik Dt

dX RC dt - physics.purdue.edu

dX RC dt - physics.purdue.edu

dx 6 dt - spbu.ru

dx 6 dt - spbu.ru

Cosmology with WFMOS

Cosmology with WFMOS

Standard Cosmology II - Istituto Nazionale di Fisica Nucleare

Standard Cosmology II - Istituto Nazionale di Fisica Nucleare

String Gas Cosmology - arXiv.org e-Print archive ·  · 2008-08-06String Gas Cosmology 5 In the best possible world, the initial phase of string cosmology will eliminate the cosmological

String Gas Cosmology - arXiv.org e-Print archive ·  · 2008-08-06String Gas Cosmology 5 In the best possible world, the initial phase of string cosmology will eliminate the cosmological

Motivic -functionsbloch/new_motivic_gamma_talk.pdf(3;2) = X m>n 1 1 m3n2 = Z 1 0 dt t dt t dt 1 t dt t dt 1 t: Remark: For the iterated integral of a MZV to converge, we must have

Motivic -functionsbloch/new_motivic_gamma_talk.pdf(3;2) = X m>n 1 1 m3n2 = Z 1 0 dt t dt t dt 1 t dt t dt 1 t: Remark: For the iterated integral of a MZV to converge, we must have

Basic concepts in DT systems - UVicaalbu/elec310_2009/ELEC 310-4-Basic...Alexandra Branzan Albu ELEC 310-Spring 2009-Lecture 4 5 Periodicity properties of DT •CT x(t) =e jω 0 t

Basic concepts in DT systems - UVicaalbu/elec310_2009/ELEC 310-4-Basic...Alexandra Branzan Albu ELEC 310-Spring 2009-Lecture 4 5 Periodicity properties of DT •CT x(t) =e jω 0 t

Is cosmology a solved problem?

Is cosmology a solved problem?

Lecture 9 Observational Cosmology Discovery of “Dark Energy”

Lecture 9 Observational Cosmology Discovery of “Dark Energy”

PROBING THE INHOMOGENEOUS UNIVERSE WITH GW COSMOLOGY …tamago.mtk.nao.ac.jp/decigo/File/international/amaldi9_20110710... · PROBING THE INHOMOGENEOUS UNIVERSE WITH GW COSMOLOGY

PROBING THE INHOMOGENEOUS UNIVERSE WITH GW COSMOLOGY …tamago.mtk.nao.ac.jp/decigo/File/international/amaldi9_20110710... · PROBING THE INHOMOGENEOUS UNIVERSE WITH GW COSMOLOGY