Evidence of 176Hf excess in select meteorites older than 4556Ma was suggested to be caused by excitation of long-lived natural radionuclide 176Lu to its short-lived isomer 176mLu, due to an irradiation event during accretion in the early solar system. A
International audienceUnderstanding the origin of volatile element variations in the inner Solar Sys...
The short-lived radionuclide, 182Hf (t1/2 = 8.9 million years) decays to 182W (natural abundance 26%...
New precise Te isotope data acquired by multiple collector inductively coupled plasma mass spectrome...
Evidence of <sup>176</sup>Hf excess in select meteorites older than 4556Ma was suggested to be cause...
Studies of Lu-Hf isotope systematics in meteorites have produced apparent "ages" that are older than...
The long-lived (176) Lu-(176) Hf and Sm-147-Nd-143 radioisotope systems are commonly used chronomete...
[[abstract]]Because La-138 is rare, refractory, and of peculiar nucleosynthetic origin, we have atte...
Knowledge of planetary differentiation is crucial for understanding the chemical and thermal evoluti...
The use of radioactive decay of 176Lu to 176Hf to study the evolution of the Earth requires a precis...
International audienceWhen recent geological calibrations of the 176Lu decay constant are used, the ...
The application of the lutetium-176/hafnium-176 method to gram quantities of minerals containing rar...
Aqueous processes were important modifiers of solid matter during the early stages of solar system h...
Aqueous processes were important modifiers of solid matter during the early stages of solar system h...
International audienceSignificance 146 Sm- 142 Nd radioactive systematics can provide constraints on...
The half-life of 176Lu was determined by measuring the 176Lu activity in metallic lutetium foils. Th...
International audienceUnderstanding the origin of volatile element variations in the inner Solar Sys...
The short-lived radionuclide, 182Hf (t1/2 = 8.9 million years) decays to 182W (natural abundance 26%...
New precise Te isotope data acquired by multiple collector inductively coupled plasma mass spectrome...
Evidence of <sup>176</sup>Hf excess in select meteorites older than 4556Ma was suggested to be cause...
Studies of Lu-Hf isotope systematics in meteorites have produced apparent "ages" that are older than...
The long-lived (176) Lu-(176) Hf and Sm-147-Nd-143 radioisotope systems are commonly used chronomete...
[[abstract]]Because La-138 is rare, refractory, and of peculiar nucleosynthetic origin, we have atte...
Knowledge of planetary differentiation is crucial for understanding the chemical and thermal evoluti...
The use of radioactive decay of 176Lu to 176Hf to study the evolution of the Earth requires a precis...
International audienceWhen recent geological calibrations of the 176Lu decay constant are used, the ...
The application of the lutetium-176/hafnium-176 method to gram quantities of minerals containing rar...
Aqueous processes were important modifiers of solid matter during the early stages of solar system h...
Aqueous processes were important modifiers of solid matter during the early stages of solar system h...
International audienceSignificance 146 Sm- 142 Nd radioactive systematics can provide constraints on...
The half-life of 176Lu was determined by measuring the 176Lu activity in metallic lutetium foils. Th...
International audienceUnderstanding the origin of volatile element variations in the inner Solar Sys...
The short-lived radionuclide, 182Hf (t1/2 = 8.9 million years) decays to 182W (natural abundance 26%...
New precise Te isotope data acquired by multiple collector inductively coupled plasma mass spectrome...