4,320 research outputs found
Vitreous GeO2 response to shock loading
Shock wave profiles in vitreous GeO2 (6.56 Mg/m^3) under planar loading were measured using stress gauges to 14 GPa. New and previous data yield Hugoniot: D=0.974 (km/s)+1.711 u for shocks of 6 to 40 GPa. We show that the phase change from 4- to 6-fold coordination of Ge+4 with O–2 in vitreous GeO2 occurs from 4 to 15 GPa. Hugoniots of vitreous GeO2 and SiO2 are found to approximately coincide if the pressure in SiO2 is scaled by the ratio of SiO2 to GeO2 initial density
Spin effects in strong-field laser-electron interactions
The electron spin degree of freedom can play a significant role in
relativistic scattering processes involving intense laser fields. In this
contribution we discuss the influence of the electron spin on (i) Kapitza-Dirac
scattering in an x-ray laser field of high intensity, (ii) photo-induced
electron-positron pair production in a strong laser wave and (iii) multiphoton
electron-positron pair production on an atomic nucleus. We show that in all
cases under consideration the electron spin can have a characteristic impact on
the process properties and their total probabilities. To this end,
spin-resolved calculations based on the Dirac equation in the presence of an
intense laser field are performed. The predictions from Dirac theory are also
compared with the corresponding results from the Klein-Gordon equation.Comment: 9 pages, 6 figure
Influência do espaçamento na produção volumétrica e qualidade da madeira de Mimosa scabrella Benth. e Eucalyptus viminalis Labill.
bitstream/item/101160/1/PA-1983-Ahrens-InfluenciaEspacamentoProducao.pdf.pd
A previsão normativa para o pagamento por serviços ambientais no código florestal brasileiro.
Neste capÃtulo documenta-se uma análise introdutória acerca do tratamento propiciado ao pagamento por serviços ambientais (PSAs) no Código Florestal brasileiro, reformado com a edição da Lei nº 12.651/2012 (BRASIL, 2012). Em seu art. 41, aquela Lei estabelece que o poder público federal poderá instituir um programa de apoio e incentivo à conservação do meio ambiente, prevendo-se, no inciso I, a possibilidade de se promover PSAs como retribuição à s atividades de conservação e melhoria de ecossistemas nos casos nominados: sistemas produtivos agrÃcolas. Todavia, são contemplados no inciso II, do mesmo artigo, que trata da obtenção de crédito agrÃcola, com taxas de juros menores, e da contratação de seguro agrÃcola em condições mais favoráveis que as praticadas no mercado. De outro lado, por se tratar de norma programática, e para que tenha efetividade, o art. 41 ainda requer regulamentação, o que se recomenda.CapÃtulo 31
Efeitos da primeira poda em povoamentos jovens de Pinus elliottii var elliottii, estabelecidos na região costeira do Rio Grande do Sul.
bitstream/item/101229/1/PA-1983-Ahrens-EfeitosPrimeira.pd
Efeitos da primeira poda em povoamentos jovens de Pinus taeda L. estabelecidos em Mafra, SC, região do alto rio negro.
bitstream/item/101227/1/PA-1983-Abrens-EfeitoPrimeira.pd
From AMANDA to IceCube
The first string of the neoteric high energy neutrino telescope IceCube
successfully began operating in January 2005. It is anticipated that upon
completion the new detector will vastly increase the sensitivity and extend the
reach of AMANDA to higher energies. A discussion of the IceCube's discovery
potential for extra-terrestrial neutrinos, together with the prospects of new
physics derived from the ongoing AMANDA research will be the focus of this
paper. Preliminary results of the first antarctic high energy neutrino
telescope AMANDA searching in the muon neutrino channel for localized and
diffuse excess of extra-terrestrial neutrinos will be reviewed using data
collected between 2000 and 2003. Neutrino flux limits obtained with the
all-flavor dedicated UHE and cascade analyses will be described. A first
neutrino spectrum above one TeV in agreement with atmospheric neutrino flux
expectations and no extra-terrestrial contribution will be presented, followed
by a discussion of a limit for neutralino CDM candidates annihilating in the
center of the Sun.Comment: 15 pages, 8 figures Invited talk contribution at 5th International
Conference on Non-accelerator New Physics (NANP 05), Dubna, Russia, 20-25 Jun
200
Extremely energetic cosmic neutrinos: Opportunities for astrophysics, particle physics, and cosmology
Existing and planned observatories for cosmic neutrinos open up a huge window
in energy from 10^7 to 10^17 GeV. Here, we discuss in particular the
possibilities to use extremely energetic cosmic neutrinos as a diagnostic of
astrophysical processes, as a tool for particle physics beyond the Standard
Model, and as a probe of cosmology.Comment: 10 pages, 7 figures, ws-procs9x6.cls, talk presented at the ARENA
Workshop, DESY, Zeuthen, Germany, May 17-19, 200
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