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1.
Phys Rev Lett ; 112(19): 192501, 2014 May 16.
Artigo em Inglês | MEDLINE | ID: mdl-24877933

RESUMO

The neutron capture cross sections of the main uranium isotopes, (235)U and (238)U, were measured simultaneously for keV energies, for the first time by combining activation technique and atom counting of the reaction products using accelerator mass spectrometry. New data, with a precision of 3%-5%, were obtained from mg-sized natural uranium samples for neutron energies with an equivalent Maxwell-Boltzmann distribution of kT ∼ 25 keV and for a broad energy distribution peaking at 426 keV. The cross-section ratio of (235)U(n,γ)/(238)U(n,γ) can be deduced in accelerator mass spectrometry directly from the atom ratio of the reaction products (236)U/(239)U, independent of any fluence normalization. Our results confirm the values at the lower band of existing data. They serve as important anchor points to resolve present discrepancies in nuclear data libraries as well as for the normalization of cross-section data used in the nuclear astrophysics community for s-process studies.

2.
Proc Natl Acad Sci U S A ; 104(41): 16016-21, 2007 Oct 09.
Artigo em Inglês | MEDLINE | ID: mdl-17901202

RESUMO

A carbon-rich black layer, dating to approximately 12.9 ka, has been previously identified at approximately 50 Clovis-age sites across North America and appears contemporaneous with the abrupt onset of Younger Dryas (YD) cooling. The in situ bones of extinct Pleistocene megafauna, along with Clovis tool assemblages, occur below this black layer but not within or above it. Causes for the extinctions, YD cooling, and termination of Clovis culture have long been controversial. In this paper, we provide evidence for an extraterrestrial (ET) impact event at approximately equal 12.9 ka, which we hypothesize caused abrupt environmental changes that contributed to YD cooling, major ecological reorganization, broad-scale extinctions, and rapid human behavioral shifts at the end of the Clovis Period. Clovis-age sites in North American are overlain by a thin, discrete layer with varying peak abundances of (i) magnetic grains with iridium, (ii) magnetic microspherules, (iii) charcoal, (iv) soot, (v) carbon spherules, (vi) glass-like carbon containing nanodiamonds, and (vii) fullerenes with ET helium, all of which are evidence for an ET impact and associated biomass burning at approximately 12.9 ka. This layer also extends throughout at least 15 Carolina Bays, which are unique, elliptical depressions, oriented to the northwest across the Atlantic Coastal Plain. We propose that one or more large, low-density ET objects exploded over northern North America, partially destabilizing the Laurentide Ice Sheet and triggering YD cooling. The shock wave, thermal pulse, and event-related environmental effects (e.g., extensive biomass burning and food limitations) contributed to end-Pleistocene megafaunal extinctions and adaptive shifts among PaleoAmericans in North America.


Assuntos
Planeta Terra , Extinção Biológica , Meteoroides , Animais , Carbono/análise , Clima , Ecossistema , Fenômenos Geológicos , Geologia , Humanos , Gelo/análise , Irídio/análise , Magnetismo , Modelos Teóricos , América do Norte , Fenômenos Físicos , Física , Solo/análise , Radioisótopos de Tálio/análise , Fatores de Tempo , Urânio/análise
3.
Phys Rev Lett ; 93(14): 142504, 2004 Oct 01.
Artigo em Inglês | MEDLINE | ID: mdl-15524787

RESUMO

Radiative strength functions (RSFs) for the (56,57)Fe nuclei below the separation energy are obtained from the 57Fe(3He,alphagamma)56Fe and 57Fe(3He,3He'gamma)57Fe reactions, respectively. An enhancement of more than a factor of 10 over common theoretical models of the soft (E(gamma) less than or approximately equal 2 MeV) RSF for transitions in the quasicontinuum (several MeV above the yrast line) is observed. Two-step cascade intensities with soft primary transitions from the 56Fe(n,2gamma)57Fe reaction confirm the enhancement.

4.
Appl Radiat Isot ; 57(4): 573-7, 2002 Oct.
Artigo em Inglês | MEDLINE | ID: mdl-12361337

RESUMO

A second cold-neutron beam experimental station has been built as part of the renewal of the PGAA facility of the Budapest Research Reactor. This new station has been instrumented for neutron-induced prompt gamma-ray spectroscopy, involving gamma-gamma coincidence measurements. The experimental setup is discussed, and its performance and our data analysis method in a case of a radioactive source coincidence experiment are presented.

5.
Appl Radiat Isot ; 56(3): 535-41, 2002 Mar.
Artigo em Inglês | MEDLINE | ID: mdl-11922421

RESUMO

Applicability of the gamma-gamma regional coincidence method to prompt gamma activation analysis has been examined in a series of model experiments. It is shown that the requirement of coincidence with a spectral range instead of a single peak greatly improves the signal to background ratio, yet preserves the linear relationship between concentration and analytical signal. The method is especially suitable for trace analysis of solutions containing hydrogen, and of matrices containing boron or other strong single gamma-ray emitters.

6.
Appl Radiat Isot ; 53(4-5): 527-33, 2000 Oct.
Artigo em Inglês | MEDLINE | ID: mdl-11003487

RESUMO

A new catalogue of subthermal neutron-induced prompt gamma rays has been created for 79 elements, from hydrogen to uranium (including fission), on the basis of recent measurements at the Budapest guided-neutron PGAA facility. New energy values have been measured using 35Cl neutron-capture gamma rays, while the gamma-ray production cross-sections have been determined with respect to the 1H thermal capture cross-section. The elemental data have been compared with thermal neutron-capture data for individual nuclides from the Evaluated Nuclear Structure Data File, ENSDF, hence isotope identifications could be made. The catalogue contains elemental spectra and a table with nearly 7000 gamma rays with relative intensity over 1% of the strongest line. The average accuracy is about 0.08 keV for energies and about 5% for cross-sections in the whole energy range, from about 40 keV to 11 MeV.

8.
Phys Rev Lett ; 76(8): 1208-1211, 1996 Feb 19.
Artigo em Inglês | MEDLINE | ID: mdl-10061663
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