Rowley, J., Compton, N., Djalali, C., Hicks, K., Price, J., Zachariou, N., … CLAS Collaboration. (2021). Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0  GeV/c as a Main Ingredient of the Neutron Star Equation of State. Physical Review Letters, 127(27), 272303. https://doi.org/10.1103/physrevlett.127.272303

Rowley, J., N. Compton, C. Djalali, K. Hicks, J. Price, N. Zachariou, K. P. Adhikari, et al. “Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0  GeV/c as a Main Ingredient of the Neutron Star Equation of State.” Physical Review Letters 127, no. 27 (December 2021): 272303. https://doi.org/10.1103/physrevlett.127.272303.

Rowley J, Compton N, Djalali C, Hicks K, Price J, Zachariou N, et al. Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0  GeV/c as a Main Ingredient of the Neutron Star Equation of State. Physical review letters. 2021 Dec;127(27):272303.

Rowley, J., et al. “Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0  GeV/c as a Main Ingredient of the Neutron Star Equation of State.” Physical Review Letters, vol. 127, no. 27, Dec. 2021, p. 272303. Epmc, doi:10.1103/physrevlett.127.272303.

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