J. S. Randhawa

collaborators

4 papers

nucl-ex2026

Detailed Study of the $^{59}$ Cu(p, $I^\pm)^{56}$ Ni Reaction and Constraints on Its Astrophysical Reaction Rate

E. Lopez-Saavedra, M. L. Avila, W. -J. Ong +20

The $^{59}$ Cu $(p, I^\pm)^{56}$ Ni reaction plays an important role in explosive astrophysical scenarios such as Type I X-ray bursts and the $I^½ p$ -process in neutrino-driven winds follow…

nucl-ex2026

Direct Measurement of the $^{59}$ Cu $(p, I^\pm)^{56}$ Ni Excitation Function to Constrain the Ni--Cu Cycle Strength and Its Impact on Explosive Nucleosynthesis

E. Lopez-Saavedra, M. L. Avila, W. -J. Ong +21

A new direct measurement of the 59Cu(p,a)56Ni excitation function from 2.43-5.88 MeV in the center-of-mass was performed in inverse kinematics using the high-efficiency MUSIC activ…

astro-ph.HE2025

Direct measurement of $^{59}$ Cu( $p$ , $I^\pm$ ) $^{56}$ Ni precludes a strong NiCu cycle in Type-I X-ray bursts

N. Bhathi, J. S. Randhawa, R. Kanungo +36

Model-observation comparisons of type-I X-ray bursts (XRBs) can reveal the properties of accreting neutron star systems, including the neutron star compactness. XRBs are powered by…

astro-ph.HE2025

Enhanced Nuclear Binding Near the Proton Dripline Opens Possible Bypass of the $^{64} Ge$ rp-process Waiting Point

Z. Meisel, W. -J. Ong, J. S. Randhawa

We performed astrophysics model calculations with updated nuclear data to identify a possible bypass of the $^{64} Ge$ waiting-point, a defining feature of the rapid-proton ca…

Detailed Study of the 59Cu(p,I^±)56Ni Reaction and Constraints on Its Astrophysical Reaction Rate

Direct Measurement of the 59Cu(p,I^±)56Ni Excitation Function to Constrain the Ni--Cu Cycle Strength and Its Impact on Explosive Nucleosynthesis

Direct measurement of 59Cu(p,I^±)56Ni precludes a strong NiCu cycle in Type-I X-ray bursts

Enhanced Nuclear Binding Near the Proton Dripline Opens Possible Bypass of the 64Ge rp-process Waiting Point

Detailed Study of the $^{59}$ Cu(p, $I^\pm)^{56}$ Ni Reaction and Constraints on Its Astrophysical Reaction Rate

Direct Measurement of the $^{59}$ Cu $(p, I^\pm)^{56}$ Ni Excitation Function to Constrain the Ni--Cu Cycle Strength and Its Impact on Explosive Nucleosynthesis

Direct measurement of $^{59}$ Cu( $p$ , $I^\pm$ ) $^{56}$ Ni precludes a strong NiCu cycle in Type-I X-ray bursts

Enhanced Nuclear Binding Near the Proton Dripline Opens Possible Bypass of the $^{64} Ge$ rp-process Waiting Point