J. P. Greene

Initial tests of Accelerator Mass Spectrometry with the Argonne Gas-Filled Analyzer and the commissioning of the MONICA detector

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>ν</mml:mi><mml:msub><mml:mi>i</mml:mi><mml:mrow><mml:mn>13</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math> structures in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Sm</mml:mi><mml:mprescripts/><mml:none/><mml:mn>155</mml:mn></mml:mmultiscripts></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi

Possible quenching of static neutron pairing near the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn>98</mml:mn></mml:mrow></mml:math> deformed shell gap: Rotational structures in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Gd</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>160</mml:mn><mml:mo>,</mml:mo><mml:mn>161</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>

Isotope harvesting at FRIB: additional opportunities for scientific discovery

Reaction rate for carbon burning in massive stars

How well do we understand the reaction rate of C burning?

Improved limit on the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Ra</mml:mi><mml:mprescripts/><mml:none/><mml:mn>225</mml:mn></mml:mmultiscripts></mml:math>electric dipole moment

Fusion measurements of¹²C+¹²C at energies of astrophysical interest

First Measurement of the Atomic Electric Dipole Moment of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>Ra</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>225</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:math>

Limit on Tensor Currents from<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>Li</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>8</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>β</mml:mi></mml:mrow></mml:math>Decay

Towards a measurement of the half-life of 60Fe for stellar and early Solar System models

Fusion of 60Ni + 100Mo near and below the Coulomb barrier

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>β</mml:mi></mml:math>-Delayed Neutron Spectroscopy Using Trapped Radioactive Ions

RETRACTED: A Shorter ¹⁴⁶ Sm Half-Life Measured and Implications for ¹⁴⁶ Sm- ¹⁴² Nd Chronology in the Solar System

Mass measurements near the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>r</mml:mi></mml:math>-process path using the Canadian Penning Trap mass spectrometer

Measurements of fusion cross-sections in 12C+12C at low beam energies using a particle-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si0010.gif" overflow="scroll"><mml:mi mathvariant="normal">γ</mml:mi></mml:math> coincidence technique

Experimental study of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow/><mml:mn>19</mml:mn></mml:msup></mml:math>O(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>d</mml:mi></mml:math>,<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi></mml:math>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow/><mml:mn>20</mml:mn></mml:msup></mm

Efficient, tightly-confined trapping of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow/><mml:mn mathvariant="bold">226</mml:mn></mml:msup></mml:math>Ra

New AMS method to measure the atom ratio 146Sm/147Sm for a half-life determination of 146Sm