Study of the A+13C interaction at heavy ION acceleration DC-60

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dc.contributor.authorMynbayev, N. A.
dc.contributor.authorGoldberg, V.Z.
dc.contributor.authorNurmukhanbetova, A.K.
dc.contributor.authorRogachev, G.V.
dc.contributor.authorGolovkov, M.S.
dc.contributor.authorDzubin, V.
dc.contributor.authorZdoroves, M.V.
dc.contributor.authorKoloberdin, M.
dc.contributor.authorIvanov, I.
dc.date.accessioned2015-11-02T06:06:47Z
dc.date.available2015-11-02T06:06:47Z
dc.date.issued2013
dc.description.abstractIn astrophysics, nuclear reactions play a great role in understanding the formation of our universe.The reaction 13C(α,n)16O is considered to be the main source of neutrons for the s process at low temperatures in low mass stars in the asymptotic giant branch. Many problems exist in analyzing this reaction using conventional experimental methods; therefore, we aimed to obtain and analyze data from the a +13C resonance elastic scattering reaction at small angles and low energies using Thick Target Inverse Kinematic method (TTIK) at heavy ion accelerator DC-60.ru_RU
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/650
dc.language.isoenru_RU
dc.publisherNazarbayev Universityru_RU
dc.subjectfirst research weekru_RU
dc.subjectastrophysicsru_RU
dc.subjectDAQ systemru_RU
dc.titleStudy of the A+13C interaction at heavy ION acceleration DC-60ru_RU
dc.typeAbstractru_RU

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