Experimental studies for the second-forbidden non-unique β-decay of 20F at IGISOL

Tähtien evoluution vaiheet perustuvat tähden alkuperäiseen massaan: kevyemmät tähdet, joiden massa on alle kahdeksan Auringon massaa päättävät evoluutionsa valkoisena kääpiönä, kun taas suuremmat tähdet, joiden massa on suurempi kuin 11 Auringon massaa päätyvät supernoviksi, jotka johtuvat tähden yt...

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Main Author: Hukkanen, Marjut
Other Authors: Matemaattis-luonnontieteellinen tiedekunta, Faculty of Sciences, Fysiikan laitos, Department of Physics, Jyväskylän yliopisto, University of Jyväskylä
Format: Master's thesis
Language:eng
Published: 2018
Subjects:
Online Access: https://jyx.jyu.fi/handle/123456789/66415
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author Hukkanen, Marjut
author2 Matemaattis-luonnontieteellinen tiedekunta Faculty of Sciences Fysiikan laitos Department of Physics Jyväskylän yliopisto University of Jyväskylä
author_facet Hukkanen, Marjut Matemaattis-luonnontieteellinen tiedekunta Faculty of Sciences Fysiikan laitos Department of Physics Jyväskylän yliopisto University of Jyväskylä Hukkanen, Marjut Matemaattis-luonnontieteellinen tiedekunta Faculty of Sciences Fysiikan laitos Department of Physics Jyväskylän yliopisto University of Jyväskylä
author_sort Hukkanen, Marjut
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description Tähtien evoluution vaiheet perustuvat tähden alkuperäiseen massaan: kevyemmät tähdet, joiden massa on alle kahdeksan Auringon massaa päättävät evoluutionsa valkoisena kääpiönä, kun taas suuremmat tähdet, joiden massa on suurempi kuin 11 Auringon massaa päätyvät supernoviksi, jotka johtuvat tähden ytimen luhistumisesta. Kuitenkin keskimassaisten tähtien evolutiivinen kaari on vielä epäselvä. On arvioitu, että keskimassaisten tähtien evoluutiossa 20Ne ytimeen taphtuvilla elektronisieppauksilla, jotka johtavat 20Fe ytimen perustilalle, on tärkeä rooli. Kuitenkin tälle perustilalta perustilalle tapahtuvan siirtymän voimakkuudelle on määritetty vain kokeellinen yläraja. Tämä työ keskittyy mittauslaitteiston, jolla mittasimme onnistuneesti kyseisen siirtymän vahvuuden ensimmäistä kertaa, kokeelliseen kehitystyöhön. Mittaukset tapahtuivat IGISOL-tutkimusryhmän tiloissa Jyväskylän yliopiston kiihdytinlaboratoriossa. 20F+-ionit tuotettiin 19F(d,p)20F reaktiolla käyttämällä 9 MeV energistä deuteronihiukkassuihkua. Kokeellinen laitteisto koostui Siegbahn-Slätis tyypin keskikuvantavasta spektrometristä, muovituikeilmaisimesta ja LaBr3(Ce)-ilmaisimesta. Tämä työ antaa kuvauksen käytetystä mittauslaitteistosta ja sen testauksesta sekä lyhyen esittelyn tähtien evoluutioon liittyvistä aiheista ja katsauksen onnistuneeseen perustilalta perustilalle tapahtuvan siirtymän mittaukseen. The evolution of stars is determined by the stars initial mass, smaller stars with masses under eight solar masses end their life as a white dwarf when the heavier stars with masses over 11 solar masses end as core-collapse supernovae. The evolutionary path of the intermediate-mass star with masses between 8 to 11 solar masses is still uncertain. The electron capture on 20Ne ground state leading to 20F ground state has been estimated to have an important role in the evolution of intermediate-mass stars. The branching of this ground-state to ground-state transition has previously had only an experimental upper limit. This thesis focuses on the experimental developments of a measurement setup which we used to measure this branching ratio for the first time. The measurement was done at the Ion Guide Isotope Separator On-Line (IGISOL) facility in the Accelerator Laboratory of the University of Jyväskylä. The 20F+ ions were produced via 19F(d,p)20F reaction with a 9 MeV deuteron beam. The experimental setup consisted of a Siegbahn-Slätis type of intermediate-image spectrometer, plastic scintillator detector and of LaBr3(Ce) detector. This work gives of a detailed description of the measurement setup and its testing as well as a brief discussion of the stellar evolution related topics and of an overview of the successful experiment.
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spellingShingle Hukkanen, Marjut Experimental studies for the second-forbidden non-unique β-decay of 20F at IGISOL stellar evolution intermediate-mass stars IGISOL beta decay SiegbanhSlätis type intermediate-image spectrometer scintillator detector tähtien evoluutio beetahajoaminen Siegbahn-Slätis tyypin keskikuvantava spektrometri tuikeilmaisin Fysiikka Physics 4021
title Experimental studies for the second-forbidden non-unique β-decay of 20F at IGISOL
title_full Experimental studies for the second-forbidden non-unique β-decay of 20F at IGISOL
title_fullStr Experimental studies for the second-forbidden non-unique β-decay of 20F at IGISOL Experimental studies for the second-forbidden non-unique β-decay of 20F at IGISOL
title_full_unstemmed Experimental studies for the second-forbidden non-unique β-decay of 20F at IGISOL Experimental studies for the second-forbidden non-unique β-decay of 20F at IGISOL
title_short Experimental studies for the second-forbidden non-unique β-decay of 20F at IGISOL
title_sort experimental studies for the second forbidden non unique β decay of 20f at igisol
title_txtP Experimental studies for the second-forbidden non-unique β-decay of 20F at IGISOL
topic stellar evolution intermediate-mass stars IGISOL beta decay SiegbanhSlätis type intermediate-image spectrometer scintillator detector tähtien evoluutio beetahajoaminen Siegbahn-Slätis tyypin keskikuvantava spektrometri tuikeilmaisin Fysiikka Physics 4021
topic_facet 4021 Fysiikka IGISOL Physics Siegbahn-Slätis tyypin keskikuvantava spektrometri SiegbanhSlätis type intermediate-image spectrometer beetahajoaminen beta decay intermediate-mass stars scintillator detector stellar evolution tuikeilmaisin tähtien evoluutio
url https://jyx.jyu.fi/handle/123456789/66415 http://www.urn.fi/URN:NBN:fi:jyu-201911184923
work_keys_str_mv AT hukkanenmarjut experimentalstudiesforthesecondforbiddennonuniquebdecayof20fatigisol