NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = M.Hernanz Found 21 matches. 2024BO08 Universe 10, 187 (2024) E.Bozzo, L.Amati, W.Baumgartner, T.-Ch.Chang, B.Cordier, N.De Angelis, A.Doi, M.Feroci, C.Froning, J.Gaskin, A.Goldstein, D.Gotz, J.E.Grove, S.Guiriec, M.Hernanz, C.M.Hui, P.Jenke, D.Kocevski, M.Kole, Ch.Kouveliotou, Th.Maccarone, M.L.McConnell, H.Matsuhara, P.O'Brien, N.Produit, P.S.Ray, P.Roming, A.Santangelo, M.Seiffert, H.Sun, A.van der Horst, P.Veres, J.Wei, N.White, C.Wilson-Hodge, D.Yonetoku, W.Yuan, Sh.-N.Zhang Future Perspectives for Gamma-ray Burst Detection from Space
doi: 10.3390/universe10040187
2017LA12 Astrophys.J. 846, 65 (2017) M.La Cognata, R.G.Pizzone, J.Jose, M.Hernanz, S.Cherubini, M.Gulino, G.G.Rapisarda, and C.Spitaleri A Trojan Horse Approach to the Production of 18F in Novae NUCLEAR REACTIONS 18F(p, α), E(cm)<1 MeV; analyzed available data using R-matrix formalism; deduced S-factors changes.
doi: 10.3847/1538-4357/aa845f
2008JO02 J.Phys.(London) G35, 014024 (2008) 10 Gyr of classical nova explosions
doi: 10..1088/0954-3899/35/1/014024
2007CH25 Phys.Rev. C 75, 035810 (2007) A.Chafa, V.Tatischeff, P.Aguer, S.Barhoumi, A.Coc, F.Garrido, M.Hernanz, J.Jose, J.Kiener, A.Lefebvre-Schuhl, S.Ouichaoui, N.de Sereville, J.-P.Thibaud Experimental determination of the 17O(p, α)14N and 17O(p, γ)18F reaction rates NUCLEAR REACTIONS 14N(α, γ), E=1620-1775 keV; measured Eγ, Iγ; deduced resonance parameters. 17O(p, α), E=194-204 keV; measured Eα, σ(E, θ); deduced resonance energy, strength. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.75.035810
2006JO08 Eur.Phys.J. A 27, Supplement 1, 107 (2006) Beacons in the sky: Classical novae vs. X-ray bursts
doi: 10.1140/epja/i2006-08-015-8
2006JO13 Nucl.Phys. A777, 550 (2006) Nucleosynthesis in classical novae
doi: 10.1016/j.nuclphysa.2005.02.121
2005CH44 Phys.Rev.Lett. 95, 031101 (2005); Erratum Phys.Rev.Lett. 96, 019902 (2006) A.Chafa, V.Tatischeff, P.Aguer, S.Barhoumi, A.Coc, F.Garrido, M.Hernanz, J.Jose, J.Kiener, A.Lefebvre-Schuhl, S.Ouichaoui, N.de Sereville, J.-P.Thibaud Hydrogen Burning of 17O in Classical Novae NUCLEAR REACTIONS 14N(α, γ), E=1775 keV; measured Eγ, Iγ. 17,18O(p, α), E ≈ 190-205 keV; measured Eα, σ, σ(θ); deduced resonance parameters. Astrophysical implications discussed.
doi: 10.1103/PhysRevLett.95.031101
2005HE20 Nucl.Phys. A758, 721c (2005) Gamma-rays from classical nova explosions: theory and observations
doi: 10.1016/j.nuclphysa.2005.05.129
2003BI03 Phys.Rev.Lett. 90, 162501 (2003); Erratum Phys.Rev.Lett. 90, 229902 (2003) S.Bishop, R.E.Azuma, L.Buchmann, A.A.Chen, M.L.Chatterjee, J.M.D'Auria, S.Engel, D.Gigliotti, U.Greife, M.Hernanz, D.Hunter, A.Hussein, D.Hutcheon, C.Jewett, J.Jose, J.King, S.Kubono, A.M.Laird, M.Lamey, R.Lewis, W.Liu, S.Michimasa, A.Olin, D.Ottewell, P.D.Parker, J.G.Rogers, F.Strieder, C.Wrede 21Na(p, γ)22Mg Reaction and Oxygen-Neon Novae NUCLEAR REACTIONS 1H(21Na, γ), E(cm) ≈ 202-223 keV; measured Eγ, (particle)γ-coin, thick-target yields; deduced resonance energy, width. 21Na(p, γ), E=low; deduced astrophysical reaction rate.
doi: 10.1103/PhysRevLett.90.162501
2003DA13 Phys.Rev. C 67, 065808 (2003) B.Davids, A.M.van den Berg, P.Dendooven, F.Fleurot, M.Hunyadi, M.A.de Huu, R.H.Siemssen, H.W.Wilschut, H.J.Wortche, M.Hernanz, J.Jose, K.E.Rehm, A.H.Wuosmaa, R.E.Segel Astrophysical rate of 15O(α, γ)19Ne via the (p, t) reaction in inverse kinematics NUCLEAR REACTIONS 1H(21Ne, t), E=43 MeV/nucleon; measured particle spectra, yields, (particle)(recoil)-coin; deduced excitation energy spectrum. 19Ne levels deduced α-decay branching widths. 15O(α, γ), E=low; deduced astrophysical reaction rates.
doi: 10.1103/PhysRevC.67.065808
2003DA36 Phys.Rev. C 68, 055805 (2003) B.Davids, J.P.M.Beijers, A.M.van den Berg, P.Dendooven, S.Harmsma, M.Hunyadi, M.A.de Huu, R.H.Siemssen, H.W.Wilschut, H.J.Wortche, M.Hernanz, J.Jose Proton-decaying states in 22Mg and the nucleosynthesis of 22Na in novae NUCLEAR REACTIONS 1H(24Mg, t), E=55 MeV/nucleon; measured particle spectra, (recoil)(triton)-coin. 22Mg deduced levels, J, π, proton-decay branching ratios. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.68.055805
2003GO24 Nucl.Phys. A718, 596c (2003) S.Goriely, J.Jose, M.Hernanz, M.Rayet, M.Arnould P-process nucleosynthesis during He-detonation in sub-Chandrasekhar CO white dwarfs
doi: 10.1016/S0375-9474(03)00879-0
2003JO12 Nucl.Phys. A718, 255c (2003) J.Jose, M.Hernanz, E.Garcia-Berro The Impact of the Chemical Stratification of White Dwarfs on the Nucleosynthesis from Classical Novae
doi: 10.1016/S0375-9474(03)00723-1
2001AM03 Nucl.Phys. A688, 430c (2001) S.Amari, E.Zinner, J.Jose, M.Hernanz Presolar Grains from Novae
doi: 10.1016/S0375-9474(01)00746-1
2001CO14 Nucl.Phys. A688, 450c (2001) A.Coc, N.Smirnova, J.Jose, M.Hernanz, J.-P.Thibaud Update of Nuclear Reaction Rates Affecting Nucleosynthesis in Novae NUCLEAR REACTIONS 21Na(p, γ), 18F(p, α), (p, γ), E=low; calculatedσ, reaction rates. Comparison with data and other theoretical calculations.
doi: 10.1016/S0375-9474(01)00752-7
2001JO13 Nucl.Phys. A688, 118c (2001) Classical Novae: Sources of CNO-model and gamma-ray emitters NUCLEAR STRUCTURE 7Be, 7Li, 22Na, 26Al, 18F; analyzed, surveyed astrophysical nuclear reaction rates; deduced nova yields, production mechanisms following network calculations.
doi: 10.1016/S0375-9474(01)00680-7
2001JO14 Nucl.Phys. A688, 439c (2001) J.Jose, M.Hernanz, S.Amari, E.Zinner Nova Outbursts and Dust Formation: Where do we stand ?
doi: 10.1016/S0375-9474(01)00749-7
2001MO21 Nucl.Phys. A688, 447c (2001) Nucleosynthesis in Accreting Neutron Stars
doi: 10.1016/S0375-9474(01)00751-5
1999HE40 Astrophys.J. 525, L97 (1999) M.Hernanz, J.Jose, A.Coc, J.Gomez-Gomar, J.Isern Gamma-Ray Emission from Novae Related to Positron Annihilation: Constraints on its observability posed by new experimental nuclear data NUCLEAR REACTIONS 18F(p, α), (p, γ), E=low; analyzed astrophysical reaction rates; deduced implications for γ-ray emission from novae.
doi: 10.1086/312372
1999JO08 Astrophys.J. 520, 347 (1999) Nuclear Uncertainties in the NeNa-MgAl Cycles and Production of 22Na and 26Al During Nova Outbursts NUCLEAR REACTIONS 21Ne, 21,22,23Na, 23,25,26,27Al, 23,26Mg, 26Si(p, γ), E not given; analyzed reaction rates, uncertainties for nova outbursts; deduced implications for 22Na, 26Al nucleosynthesis.
doi: 10.1086/307445
1997JO13 Nucl.Phys. A621, 491c (1997) Nucleosynthesis in Novae. Implications on Lithium Production and Gamma-Ray Radionuclides
doi: 10.1016/S0375-9474(97)00295-9
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