The baryon density of the Universe from an improved rate of deuterium burning
Cyburt, R. H., Fields, B. D., Olive, K. A. & Yeh, T.-H. Big Bang nucleosynthesis: present status. Rev. Mod. Phys. 88, 015004 (2016).
Tanabashi, M. et al. Review of particle physics. Phys. Rev. D 98, 030001 (2018).
Cooke, R., Pettini, M. & Steidel, C. One percent determination of the primordial deuterium abundance. Astrophys. J. 855, 102 (2018).
Pitrou, C., Coc, A., Uzan, J. & Vangioni, E. Precision Big Bang nucleosynthesis with improved helium-4 predictions. Phys. Rep. 754, 1–66 (2018).
Coc, A. et al. New reaction rates for improved primordial D/H calculation and the cosmic evolution of deuterium. Phys. Rev. D 92, 123526 (2015).
Di Valentino, E. et al. Probing nuclear rates with Planck and BICEP2. Phys. Rev. D 90, 023543 (2014).
Aghanim, N. et al. Planck 2018 results. VI. Cosmological parameters. Astron. Astrophys. 641, A6 (2020).
Broggini, C., Bemmerer, D., Caciolli, A. & Trezzi, D. LUNA: status and prospects. Prog. Part. Nucl. Phys. 98, 55–84 (2018).
Cavanna, F. & Prati, P. Direct measurement of nuclear cross-section of astrophysical interest: results and perspectives. Int. J. Mod. Phys. A 33, 1843010–1843042 (2018).
Mossa, V. et al. Setup commissioning for an improved measurement of the D(p,γ)3He cross section at Big Bang nucleosynthesis energies. Eur. Phys. J. A 56, 144 (2020).
Formicola, A. et al. The LUNA II 400kV accelerator. Nucl. Instrum. Methods Phys. Res. A 507, 609–616 (2003).
Fields, B. D., Olive, K. A., Yeh, T.-H. & Young, C. Big-Bang nucleosynthesis after Planck. J. Cosmol. Astropart. Phys. 03, 010 (2020).
Casella, C. et al. First measurement of the d(p,γ)3He cross section down to the solar Gamow peak. Nucl. Phys. A 706, 203–216 (2002).
Ma, L. et al. Measurements of 1H(d→,γ)3He and 2H(p→,γ)3He at very low energies. Phys. Rev. C 55, 588–596 (1997).
Griffiths, G., Larson, E. & Robertson, L. The capture of protons by deuterons. Can. J. Phys. 40, 402–411 (1962).
Schmid, G. et al. The 2H(p,γ)3He and 1H(d,γ)3He reactions below 80 keV. Phys. Rev. C 56, 2565–2581 (1997).
Tišma, I. et al. Experimental cross section and angular distribution of the 2H(p,γ)3He reaction at Big-Bang nucleosynthesis energies. Eur. Phys. J. A 55, 137 (2019).
Marcucci, L., Mangano, G., Kievsky, A. & Viviani, M. Implication of the proton-deuteron radiative capture for Big Bang nucleosynthesis. Phys. Rev. Lett. 116, 102501 (2016).
Adelberger, E. et al. Solar fusion cross sections. II. The pp chain and CNO cycles. Rev. Mod. Phys. 83, 195–245 (2011).
Schmid, G. et al. Effects of non-nucleonic degrees of freedom in the D(\(\overrightarrow{{p}}\),γ)3He and the p(\(\overrightarrow{{d}}\),γ)3He reactions Phys. Rev. Lett. 76, 3088–3091 (1996).
Iliadis, C., Anderson, K. S., Coc, A., Timmes, F. X. & Starrfield, S. Bayesian estimation of thermonuclear reaction rates. Astrophys. J. 831, 107 (2016).
Consiglio, R. et al. PArthENoPE reloaded. Comput. Phys. Commun. 233, 237–242 (2018).
De Salas, P. & Pastor, S. Relic neutrino decoupling with flavour oscillations revisited. J. Cosmol. Astropart. Phys. 07, 051 (2016).
Mangano, G. et al. Relic neutrino decoupling including flavour oscillations. Nucl. Phys. B 729, 221–234 (2005).
Aver, E., Olive, K. A., & Skillman, E. D. The effects of He I λ10830 on helium abundance determinations. J. Cosmol. Astropart. Phys. 07, 011 (2015).
Peimbert, A., Peimbert, M. & Luridiana, V. The primordial helium abundance and the number of neutrino families. Rev. Mex. Astron. Astrofis. 52, 419–424 (2016).
Valerdi, M., Peimbert, A., Peimbert, M. & Sixtos, A. Determination of the primordial helium abundance based on NGC 346, an H ii region of the Small Magellanic Cloud. Astrophys. J. 876, 98 (2019).
Izotov, Y. I., Thuan, T. X. & Guseva, N. G. The primordial deuterium abundance of the most metal-poor damped Lyα system. Mon. Not. R. Astron. Soc. 445, 778–793 (2014).
Griffiths, G., Lal, M. & Scarfe, C. The reaction D(p,γ)3He below 50 keV. Can. J. Phys. 41, 724–736 (1963).
Warren, J. B., Erdman, K. L., Robertson, L. P., Axen, D. A. & Macdonald, J. R. Photodisintegration of 3He near the threshold. Phys. Rev. 132, 1691–1692 (1963).
Geller, K., Muirhead, E. & Cohen, L. The 2H(p,γ)3He reaction at the breakup threshold. Nucl. Phys. A 96, 397–400 (1967).
Ferraro, F. et al. A high-efficiency gas target setup for underground experiments, and redetermination of the branching ratio of the 189.5 keV 22Ne(p,γ)23Na resonance. Eur. Phys. J. A 54, 44 (2018).
Rolfs, C. & Rodney, W. Cauldrons in the Cosmos (Univ. Chicago Press, 1988).
Serpico, P. D. et al. Nuclear reaction network for primordial nucleosynthesis: a detailed analysis of rates, uncertainties and light nuclei yields. J. Cosmol. Astropart. Phys. 2004, 010 (2004).
Nollett, K. M. & Burles, S. Estimating reaction rates and uncertainties for primordial nucleosynthesis. Phys. Rev. D 61, 123505 (2000).
Tumino, A. et al. New determination of the 2H(d,p)3H and 2H(d,n)3He reaction rates at astrophysical energies. Astrophys. J. 785, 96 (2014).
Pisanti, O. et al. PArthENoPE: public algorithm evaluating the nucleosynthesis of primordial elements. Comput. Phys. Commun. 178, 956–971 (2008).