• Corpus ID: 250144363

Radiative neutron capture reaction rates for r-process nucleosynthesis

  title={Radiative neutron capture reaction rates for r-process nucleosynthesis},
  author={Vinay Singh and Joydev Lahiri and Malay Kanti Dey and Dipankar Narayan Basu},
About half of the elements beyond iron are synthesized in stars by rapid-neutron capture process (r-process). The stellar environment provides very high neutron flux in a short time ( ∼ seconds) which is conducive for the creation of progressively neutron-rich nuclei till the waiting point is reached after which no further neutron capture reactions proceed. At this point such extremely neutron-rich nuclei become stable via β − decay. A detailed understanding of the r-process remains illusive. In… 



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    Fen Öğretiminde Kavram Yanılgıları Tespiti ve Giderilmesi
  • 2019
Radia t ion damage aag 6 our t o t h e l i t h i u m h y d r i b Bhieldta ai a r o a u l t of t he r e a c t i o n LP 8 (st* d,)H3. There i ta etvideaoa ia t he literature i a d h a t i a g both the

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