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NSR database version of April 11, 2024.

Search: Author = M.Hernanz

Found 20 matches.

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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
Citations: PlumX Metrics


2008JO02      J.Phys.(London) G35, 014024 (2008)

J.Jose, M.Hernanz

10 Gyr of classical nova explosions

doi: 10..1088/0954-3899/35/1/014024
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0468.


2006JO08      Eur.Phys.J. A 27, Supplement 1, 107 (2006)

J.Jose, M.Hernanz

Beacons in the sky: Classical novae vs. X-ray bursts

doi: 10.1140/epja/i2006-08-015-8
Citations: PlumX Metrics


2006JO13      Nucl.Phys. A777, 550 (2006)

J.Jose, M.Hernanz, C.Iliadis

Nucleosynthesis in classical novae

doi: 10.1016/j.nuclphysa.2005.02.121
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetF0757.


2005HE20      Nucl.Phys. A758, 721c (2005)

M.Hernanz, J.Jose

Gamma-rays from classical nova explosions: theory and observations

doi: 10.1016/j.nuclphysa.2005.05.129
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC0992.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


2001JO13      Nucl.Phys. A688, 118c (2001)

J.Jose, M.Hernanz, A.Coc

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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


2001MO21      Nucl.Phys. A688, 447c (2001)

F.Moreno, J.Jose, M.Hernanz

Nucleosynthesis in Accreting Neutron Stars

doi: 10.1016/S0375-9474(01)00751-5
Citations: PlumX Metrics


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
Citations: PlumX Metrics


1999JO08      Astrophys.J. 520, 347 (1999)

J.Jose, A.Coc, M.Hernanz

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
Citations: PlumX Metrics


1997JO13      Nucl.Phys. A621, 491c (1997)

J.Jose, M.Hernanz

Nucleosynthesis in Novae. Implications on Lithium Production and Gamma-Ray Radionuclides

doi: 10.1016/S0375-9474(97)00295-9
Citations: PlumX Metrics


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