Nuclear Astrophysics
Mostrando 1-10 de 10 artigos, teses e dissertações.
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1. A utilização do software Maxima no ensino por investigação da evolução estelar utilizando simulação gráfica da fusão nuclear
Resumo Tem sido tema comum, nas propostas curriculares, o estudo e experiências de observação do céu e dos principais fenômenos relacionados, a fim de possibilitar a compreensão de características da Terra, do Sol, da Lua e de outros corpos celestes. Recentemente, a proposta de BNCC (Base Nacional Curricular Comum) destaca a necessidade do ensino de a
Rev. Bras. Ensino Fís.. Publicado em: 07/01/2019
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2. Estudo sobre a identificação de hádrons em câmaras de fotoemulsão / Study about hadron identification in emulsion chambers
This work introduces the importance of photoemulsion chambers that remain in use after decades and still offer many advantages for elementary particle physics. We cite OPERA (Oscillation Project with Emulsion-tRacking Apparatus) detector that is the greatest lead photoemulsion chamber detector ever constructed as an example of its application nowadays (nine
IBICT - Instituto Brasileiro de Informação em Ciência e Tecnologia. Publicado em: 16/04/2012
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3. Aplicabilidade e validação do Geant4 para fótons e elétrons em radioterapia / GEANT4 applicability and validation to Photons and Electrons in Radiotherapy
Due to the increasing use of ionizing radiation in medical applications, in recent decades, the simulation codes for radiation interacting with matter, based on Monte Carlo Method, have been constantly adapted to applications in medical physics. TheMonte Carlo method is a statisticalmethod of numerical simulation of problems using essentially a sequence of r
IBICT - Instituto Brasileiro de Informação em Ciência e Tecnologia. Publicado em: 14/06/2011
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4. Study of nuclear reactions of astrophysics interest through the trojan horse method / Estudo de reações nucleares de interesse astrofísico utilizando o método do cavalo de tróia
Nuclear Astrophysics is the key to explain, among other things, the production of energy in stars, stellar evolution and the synthesis of chemical elements and isotopes in the Universe. In such cases, nuclear reactions are the main structure, where cross sections and reaction rates must be determined with reasonable accuracy in the laboratory. Because the ex
Publicado em: 2009
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5. Study of the interaction of mass A=8 nuclei with carbon target and of the capture reaction 8Li(p,y)9Be of astrophysical interest / Estudo da interação de núcleos de massa A=8 com alvo de carbono e da reação de captura 8Li(p,)9Be de interesse astrofísico
The measurements of the angular distributions for the elastic scatterings 12C(Li,Li) and 12C(8B,8B) reported in this work have been done in two laboratories. Those corresponding to the angular distributions for the elastic scattering 12C(8Li,8Li) were performed at two ene&ies, 20.6 MeV and 23.9 MeV, at the Pelletron Laboratory of the University of São Paulo
Publicado em: 2009
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6. Fator-S astrofísico da reação de captura de próton 8Li(p,)9Be através do estudo da reação de transferência elástica 9Be(8Li,9Be) / Astrophysic S-Factor for the proton capture reaction 8Li(p,)9Be using the study of the elastic transfer reaction 9Be(8Li,9Be)
Esse trabalho consistiu na determinação do Fator-S astrofísico da reação de captura 8Li(p,)9Be através do estudo da reação de transferência elástica 9Be(8Li,9Be)8Li. O fator espectroscópico do estado ligado 8Li+p=9Be, obtido à partir das medidas da distribuição angular da reação de transferência 9Be(8Li,9Be)8Li, foi utilizado para normalizar
Publicado em: 2009
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7. Quark matter (strangelets) from astrophysical sources and its detection by terrestrial experiments. / Matéria de quarks (strangelets) de origem astrofísica e sua detecção por experimentos terrestres
The strange quark matter hypothesis, which states that a plasma composed of quarks up, down and strange in roughly equal amounts is absolutely stable at zero pressure, has been studied for more than twenty years, both theoretically and during searches for its detection in specific experiments. If strange quark matter is indeed stable, then there could be imp
Publicado em: 2008
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8. Fator S astrofisico para a reação de captura 4He(t,g)7Li pela investigação da reação de transferência elástica no sistema 7Li + 4He / Astrophysical S factor for the 4He(t,g)7Li capture reaction by the investigation of the elastic-transfer reaction in the 7Li + 4He system
The normalization coefficient for the non-resonant part of the 3H(alpha,gama)7Li capture reaction (or alternately, the astrophysical S-factor) was obtained with the indirect method ANC (Asymptotic Normalization Coefficients). In this method the spectroscopic factor (or alternately, the ANC) is extracted from the investigation of a peripheral transfer reactio
Publicado em: 2007
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9. Studies in nuclear astrophysics using radioactive beams at the HRIBF
The availability of radioactive beams has produced great opportunities for advances in our understanding of the nucleosynthesis occurring in stellar explosions such as novae, X-ray bursts, and supernovae. At the HRIBF, we have used proton-rich beams such as 17;18F and neutron-rich beams such as 82Ge to study astrophysicallyimportant reaction rates. Large-are
Brazilian Journal of Physics. Publicado em: 2004-09
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10. Bragg-Surface diffraction (BSD) : high resolution microprobe to study ion implanted semiconductors / Forças de oscilador ponderadas e tempos de vida para os espectros de Si II, Si VIII e SI IX
The principal objective of this work is to present the weighed oscillator strengths (gf) and the lifetimes for all the eletric dipole transitions experimentally known for the íons of Si II, Si VIII VIII and Si IX. The interpretation of the calculation of these two values is for instance of fundamental importance in the astrophysics, because the silicon in y
Publicado em: 2000