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Chronological Thread 
  • From: Zoltan Mate <mate AT>
  • To: fizinfo <Fizinfo AT>
  • Subject: [Fizinfo] Atomki-szeminárium
  • Date: Tue, 28 Aug 2012 17:06:41 +0200 (CEST)
  • List-archive: <>
  • List-id: ELFT HÍRADÓ <>

Az MTA Atommagkutató Intézetének előadótermében
(Debrecen, Bem tér 18/c. 12. ép. III. em.)
2012. augusztus 30-án, csütörtökön 11:00-kor

Cristina Bordeanu

Work and results at ATOMKI for
the 3He+4He experiment, OTKA 82409 project

címmel előadást tart.
Az előadás előtt 10:30-tól tea, vendégeket szívesen látunk.

Máté Zoltán

In 1998, the astrophysical factor S34 data difference on direct capture
and activation methods [1] for the reaction rate 3He+4He and its importance
for the Standard Solar Model was the reason for a new experimental quest to
understand the discrepancy. New results introduced a new situation to
clarify: S34 variations for 'old' (before 1998) and 'new' data
(between 1998 and 2009) at higher energies, an important factor in the
theory models used for extrapolations, didn't look the same.
Theorists asked for new experimental data [2,3] in this region.
We started this project with the main goal to clarify the situation.
Here are the results.

[1] E. Adelberger et al., Rev. Mod. Phys. 70, 1265 (1998)
[2] Mohr Peter, PHYSICAL REVIEW C 79 (6), 065804 (2009)
[3] Cyburt R. H. and Davids B., PHYSICAL REVIEW C 78 (6), 064614 (2008)

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