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L. Ma et al., Phys. Rev. C 55, 588 (1997)
1997
Earlier work this paper cites.
J.W. Chen and M.J. Savage, Phys. Rev. C 60
1999
Earlier work this paper cites.
M. Viviani, A. Kievsky, L. E. Marcucci, S. Rosati and R. Schiavilla, Phys. Rev. C 61
2000
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G. Rupak, Nucl. Phys. A 678
2000
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C. Casella et al
2002
Earlier work this paper cites.
A. Lewis and S. Bridle, Phys. Rev. D 66
2002
Earlier work this paper cites.
C. Casella et al. (LUNA collaboration): Nuclear Physics A 706 (2002) 203�216
2002
Earlier work this paper cites.
A. Formicola et al. (LUNA collaboration), Nucl. Instr. and Meth. A 507 (2003) 609
2003
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2014

Di Valentino, Eleonora, Gustavino, Carlo, Lesgourgues, Julien et al.

Big Bang Nucleosynthesis (BBN) relates key cosmological parameters to the primordial abundance of light elements.

In this paper, we point out that the recent observations of Cosmic Microwave Background anisotropies by the Planck satellite and by the BICEP2 experiment constrain these parameters with such a high level of accuracy that the primordial deuterium abundance can be inferred with remarkable precision.
For a given cosmological model, one can obtain independent information on nuclear processes in the energy range relevant for BBN, which determine the eventual ^2H/H yield.
In particular, assuming the standard cosmological model, we show that a combined analysis of Planck data and of recent deuterium abundance measurements in metal-poor damped Lyman-alpha systems provides independent information on the cross section of the radiative capture reaction d(p,\gamma)^3He converting deuterium into helium.

L. Ma et al., Phys. Rev. C 55, 588 (1997)
1997
Earlier work this paper cites.
J.W. Chen and M.J. Savage, Phys. Rev. C 60
1999
Earlier work this paper cites.
M. Viviani, A. Kievsky, L. E. Marcucci, S. Rosati and R. Schiavilla, Phys. Rev. C 61
2000
Earlier work this paper cites.
G. Rupak, Nucl. Phys. A 678
2000
Earlier work this paper cites.
C. Casella et al
2002
Earlier work this paper cites.
A. Lewis and S. Bridle, Phys. Rev. D 66
2002
Earlier work this paper cites.
C. Casella et al. (LUNA collaboration): Nuclear Physics A 706 (2002) 203�216
2002
Earlier work this paper cites.
A. Formicola et al. (LUNA collaboration), Nucl. Instr. and Meth. A 507 (2003) 609
2003
Earlier work this paper cites.

P. D. Serpico, S. Esposito, F. Iocco, G. Mangano, G. Miele and O. Pisanti, JCAP 0412
2004
Cited alongside, same era.
L. E. Marcucci, M. Viviani, R. Schiavilla, A. Kievsky and S. Rosati, Phys. Rev. C 72
2005
Cited alongside, same era.
G. Mangano, G. Miele, S. Pastor, T. Pinto, O. Pisanti and P. D. Serpico, Nucl. Phys. B 729
2005
Cited alongside, same era.
L. E. Marcucci, K. M. Nollett, R. Schiavilla and R. B. Wiringa, Nucl. Phys. A 777
2006
Cited alongside, same era.
D.S. Leonard et al
2006
Cited alongside, same era.
O. Pisanti, A. Cirillo, S. Esposito, F. Iocco, G. Mangano, G. Miele and P. D. Serpico, Comput. Phys. Commun. 178
Original
2008
Cited alongside, same era.