Area of research
Nuclear and High Energy Physics · Radiation
Research interest
Research topics from publications: Observation of a Near-Threshold Proton Resonance in B11; Experimental study of the F17+C12 fusion reaction and its implications for fusion of proton-halo systems; The Encore active target detector: A Multi-Sampling Ionization Chamber; Resolution of a long-standing discrepancy in the $$^{17}$$O$$+^{12}$$C fusion excitation function; Low-lying resonances in Si26 relevant for the determination of the astrophysical Al25(p,γ<mml; Development of an Isomeric beam of26Al for nuclear reaction studies; Characterization of the CATRiNA neutron detector system; Experimental study of the Nam24(d,p)Na25 reaction and implications for the influence of the <m; Characterization and description of a spectrum unfolding method for the CATRiNA neutron detector array; Experimental study of the isomeric state in N16 using the Ng,m16</. Representative work: A near-threshold proton resonance in $^{11}\mathrm{B}$ at ${E}_{\mathrm{ex}}=11.44\ifmmode\pm\else\textpm\fi{}0.04\text{ }\text{ }\mathrm{MeV}$ is observed via the reaction $^{10}\mathrm{Be}(d,n)^{11}\mathrm{Be}\ensuremath{\rightarrow}^{10}\mathrm{Be}+p$ in inverse kinematics, measured with a beam of the radioactive isotope $^{10}\mathrm{Be}$. The resonance energy at ${E}_{\mathrm{res}}=211(40)\text{ }\text{ }\mathrm{keV}$ is consistent with a proton signal observed by Ayyad et al. in the $\ensuremath{\beta}$-delayed proton decay of $^{11}\mathrm{Be}$. By comparison to a distorted wave Born approximation calculation, a 0.27(6) spectroscopic factor is extracted and a tentative ($\ensuremath{\ The total fusion cross section for the $^{17}\mathrm{F}+^{12}\mathrm{C}$ system at incident energies near the top of the Coulomb barrier was studied using the newly developed Encore active-target detector at Florida State University. The $^{17}\mathrm{F}$ nucleus exhibits interesting nuclear structure properties in that although it has a low threshold against $^{17}\mathrm{F}\ensuremath{\rightarrow}^{16}\mathrm{O}+p$ breakup $({S}_{p}=600\phantom{\rule{0.28em}{0ex}}\mathrm{keV})$, the valence proton is in the $1{d}_{5/2}$ shell in the ground state so that the nuclear matter radius is predicted to be similar to that of the $^{16}\mathrm{O}$ core. By contrast, the low-lying $1/{2}^{+}$ first e
Observation of a Near-Threshold Proton Resonance in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">B</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>11</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:math>
Low-lying resonances in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Si</mml:mi><mml:mprescripts/><mml:none/><mml:mn>26</mml:mn></mml:mmultiscripts></mml:math> relevant for the determination of the astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Al</mml:mi><mml:mprescripts/><mml:none/><mml:mn>25</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mrow><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml
Characterization and description of a spectrum unfolding method for the CATRiNA neutron detector array
Experimental study of the isomeric state in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">N</mml:mi><mml:mprescripts/><mml:none/><mml:mn>16</mml:mn></mml:mmultiscripts></mml:math> using the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">N</mml:mi><mml:none/><mml:mrow><mml:mi>g</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mn>16</mml:mn></
Experimental study of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">F</mml:mi><mml:mprescripts/><mml:none/><mml:mn>17</mml:mn></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>12</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> fusion reaction and its implications for fusion of proton-halo systems
The Encore active target detector: A Multi-Sampling Ionization Chamber
Resolution of a long-standing discrepancy in the $$^{17}$$O$$+^{12}$$C fusion excitation function
Experimental study of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Na</mml:mi><mml:none/><mml:mi>m</mml:mi><mml:mprescripts/><mml:none/><mml:mn>24</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Na</mml:mi><mml:mprescripts/><mml:none/><mml:mn>25</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction and implications for the influence of the <m
Fusion-induced fission measurements with the MUSIC active target detector
Characterization of the CATRiNA neutron detector system
Development of an Isomeric beam of26Al for nuclear reaction studies
Nuclear Astrophysics Studies with an Isomeric <sup>26</sup>Al<i><sup>m</sup></i> Beam