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A. S. Botvina

Researcher at Frankfurt Institute for Advanced Studies

Publications -  135
Citations -  2711

A. S. Botvina is an academic researcher from Frankfurt Institute for Advanced Studies. The author has contributed to research in topics: Nucleon & Neutron. The author has an hindex of 29, co-authored 126 publications receiving 2515 citations. Previous affiliations of A. S. Botvina include Russian Academy of Sciences & University of Mainz.

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Multifragmentation of spectators in relativistic heavy-ion reactions

TL;DR: In this article, the authors used the ALADIN forward-spectrometer at SIS to study multi-fragment decays of 197 Au projectiles after collisions with C, Al, Cu and Pb targets at a bombarding energy of 600 MeV.
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Thermodynamical features of multifragmentation in peripheral Au + Au Collisions at 35 A.MeV

TL;DR: In this paper, the distribution of fragments produced in events involving the multifragmentation of excited sources is studied for peripheral Au + Au reactions at 35 A MeV and an isotropic emission in its rest frame has been observed, indicating that an equilibrated system has been formed.
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Multifragment break-up of nuclei by intermediate-energy protons

TL;DR: In this article, a cascade-fragmentation-evaporation (CFE) model of proton-nucleus reactions at intermediate energies is developed within the framework of this model, and a systematic analysis has been performed of a broad set of data on nuclear fragmentation induced by protons with energies E p ≈ 1-100 GeV.
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Thermodynamical features of multifragmentation in peripheral Au + Au Collisions at 35 A.MeV

TL;DR: In this paper, the distribution of fragments produced in events involving the multifragmentation of excited sources is studied for peripheral Au + Au reactions at 35 A.MeV and a temperature 4 - 6 MeV, depending on the freeze-out hypothesis.
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Statistical approach for supernova matter

TL;DR: In this paper, a statistical approach for description of nuclear composition and equation of state of stellar matter at subnuclear densities and temperature up to 20 MeV was proposed, which is expected during the collapse and explosion of massive stars.