Download - Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II
![Page 1: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/1.jpg)
Hartmut Abele 1
WMAP of cosmic 3K microwaveradiation
Staus: 300000 years after BB
Kosmologie II
![Page 2: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/2.jpg)
Hartmut Abele 2
Phase Transitions of the Universe and observables from neutron experiments The neutron as an object: ~ as a tool: New Physics: Standard Model:
Temperature 10+19 GeV Planck
GUTs - - Inflation Electroweak Chiral transition Nucleon freeze out Nuclear freeze out Atomic freeze out Galactic freeze out
10-11 GeV 10-43s 10-35s 10-12s 1 s 105y 109y today
Time
EDMMdn
qn
n nbar
mWR,
Vud
gA / gV
n
-1
N
aW
M
A ,P
, , , , ,
pp
Dubbers: ESS presentation 2002
![Page 3: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/3.jpg)
Hartmut Abele 3
![Page 4: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/4.jpg)
Hartmut Abele 4
![Page 5: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/5.jpg)
Hartmut Abele 5
![Page 6: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/6.jpg)
Hartmut Abele 6
![Page 7: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/7.jpg)
Hartmut Abele 7
blau:2.721 K
rot: 2.729 K
![Page 8: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/8.jpg)
Hartmut Abele 8
![Page 9: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/9.jpg)
Hartmut Abele 9
![Page 10: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/10.jpg)
Hartmut Abele 10
![Page 11: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/11.jpg)
Hartmut Abele 11
![Page 12: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/12.jpg)
Hartmut Abele 12
![Page 13: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/13.jpg)
Hartmut Abele 13
![Page 14: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/14.jpg)
Hartmut Abele 14
![Page 15: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/15.jpg)
Hartmut Abele 15
![Page 16: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/16.jpg)
Hartmut Abele 16
![Page 17: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/17.jpg)
Hartmut Abele 17
![Page 18: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/18.jpg)
Hartmut Abele 18
![Page 19: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/19.jpg)
Hartmut Abele 19
![Page 20: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/20.jpg)
Hartmut Abele 20
![Page 21: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/21.jpg)
Hartmut Abele 21
![Page 22: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/22.jpg)
Hartmut Abele 22
![Page 23: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/23.jpg)
Hartmut Abele 23
Nature, 17.6.05Nature, 17.6.05
![Page 24: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/24.jpg)
Hartmut Abele 24
![Page 25: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/25.jpg)
Hartmut Abele 25
![Page 26: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/26.jpg)
Hartmut Abele 26
GUTMPL
MnPL
quantum gravity
= 1/137
100 GeV, LEP-energy at CERN
= 1/128
![Page 27: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/27.jpg)
Hartmut Abele 27
![Page 28: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/28.jpg)
Hartmut Abele 28
The Neutron Lifetime and Big Bang Nucleo SynthesisThe Neutron Lifetime and Big Bang Nucleo Synthesis
Problem 1s after Big Bang:– What does a gas of n and p, when
the universe expands and the temperature drops?
Inputs:– neutron lifetime
– Cross sections– neutrino cross-sections 1/ – nuclear physics 0.1 – 1 MeV
(measured!)
Outputs: H, D, He, Li– number of particle families N
– density of (ordinary) matter in universe
![Page 29: Hartmut Abele 1 WMAP of cosmic 3K microwaveradiation Staus: 300000 years after BB Kosmologie II](https://reader036.vdocuments.mx/reader036/viewer/2022062618/55144fa4550346494e8b5087/html5/thumbnails/29.jpg)
Hartmut Abele 29