astrophysics i, lecture slides – chapter 5, eth zurich...slides5_v1_astrophysics_1_hs2019 author...
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![Page 1: Astrophysics I, Lecture Slides – Chapter 5, ETH Zurich...Slides5_v1_Astrophysics_1_HS2019 Author H.M. Schmid Created Date 10/21/2019 10:07:14 AM](https://reader034.vdocuments.us/reader034/viewer/2022051900/5fee8dc86ae7115c872676e3/html5/thumbnails/1.jpg)
Nuclear binding energy
(from Choudhuri)
Astrophysics I, Lecture Slides – Chapter 5, ETH Zurich
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Nuclear reactionrates
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Table of nuclides - type of decay
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Table of nuclides – nuclei lifetime
http://www.nndc.bnl.gov/chart4
![Page 5: Astrophysics I, Lecture Slides – Chapter 5, ETH Zurich...Slides5_v1_Astrophysics_1_HS2019 Author H.M. Schmid Created Date 10/21/2019 10:07:14 AM](https://reader034.vdocuments.us/reader034/viewer/2022051900/5fee8dc86ae7115c872676e3/html5/thumbnails/5.jpg)
Nuclear reaction, pp-chain and CNO cycle
Figure from http://www.ims.uaf.edu/isotopes/class-images/isotope-table.jpg5
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Hydrogen burning: pp-chain vs CNO-cycle
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Solar neutrino flux
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Stellar evolution in the HR-diagram
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Evolution of a 1 MS-star- HHe burning (main seq.), 9·109y,- evolution towards red giants- He-burning, 109J,- Extended red giatns with
pulsations and heavy mass loss - hot nucleous with planetary nebula- white dwarf, cooling >> 109 y.
Evolution of a 15 MS-star- HHe burning (main seq.), 2·107y- Evolution towards red giant and
strong mass loss,- He, C, O, Si burning, 106 y,- formation of Fe-core,- Core-collapse and supernova-
explosion (for stars with M > 8 MS).
HeC,O
HeC,O
O,SiFeSN
red giants
hotsubdwarfs
whitedwarfs
4.0
4.0
2.0
0.0
4.5 3.5Log T
1Ms
15Ms
Log
L/L S
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Stellar modelcalculations
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Planetary nebulae with central star
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Supernova remnant (Crab nebula)
11HST image, NASA/ESA
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Supernova 1987ASN 1987A in the Large Magellanic Cloud (50 kpc), before and after…
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Bolometric light curve of SN 1987A
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Short gamma ray burstGW170817
neutron star merger
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