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NSR database version of April 29, 2024.

Search: Author = N.Prantzos

Found 13 matches.

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2020PR16      Mon.not.R.Astron.Soc. 491, 1832 (2020)

N.Prantzos, C.Abia, S.Cristallo, M.Limongi, A.Chieffi

Chemical evolution with rotating massive star yields II. A new assessment of the solar s- and r- process components

NUCLEAR REACTIONS ⁷⁰Ge, ⁷⁶Se, ^80,82Kr, ^86,87Sr, ⁹⁶Mo, ¹⁰⁰Ru, ¹⁰⁴Pd, ¹¹⁰Cd, ¹¹⁶Sn, ^122,123,124Te, ^128,130Xe, ^134,136Ba, ¹⁴²Nd, ^148,150Sm, ¹⁵⁴Gd, ¹⁶⁰Dy, ¹⁷⁰Yb, ¹⁷⁶Lu, ¹⁷⁶Hf, ¹⁸⁶Os, ¹⁹²Pt, ¹⁹⁸Hg, ²⁰⁴Pb(n, γ), E ∼ 30 keV; analyzed available s-process only data; calculated s-process abundances.

NUCLEAR REACTIONS ^69,71Ga, ^{70,72,73,74,76}Ge, ⁷⁵As, ^{76,77,78,80,82}Se, ^79,81Br, ^{80,82,83,84,86}Kr, ^85,87Rb, ^86,87,88Sr, ⁸⁹Y, ^{90,91,92,94,96}Zr, ⁹³Nb, ^{95,96,97,98,100}Mo, ^{99,100,101,102,104}Ru, ¹⁰³Rh, ^{104,105,106,108,110}Pd, ^107,109Ag, ^{110,111,112,113,114,116}Cd, ¹¹⁵In, ^{116,117,118,119,120,122,124}Sn, ^121,123Sb, ^{122,123,124,125,126,128,130}Te, ¹²⁷I, ^{128,129,130,131,132,134,136}Xe, ¹³³Cs, ^{134,135,136,137,138}Ba, ¹³⁹La, ^140,142Ce, ¹⁴¹Pr, ^{142,143,144,145,146,148,150}Nd, ^{147,148,149,150,152,154}Sm, ^151,153Eu, ^{154,155,156,157,158,160}Gd, ¹⁵⁹Tb, ^{160,161,162,163,164}Dy, ¹⁶⁵Ho, ^{166,167,169,170}Er, ¹⁶⁹Tm, ^{170,171,172,173,174,176}Yb, ^175,176Lu, ^{176,177,178,179,180}Hf, ¹⁸¹Ta, ^{182,183,184,186}W, ^185,187Re, ^{186,187,188,189,190,192}Os, ^191,193Ir, ^{192,194,195,196,198}Pt, ¹⁹⁷Au, ^{198,199,200,201,202,204}Hg, ^203,205Tl, ^{204,206,207,208}Pb, ²⁰⁹Bi, ²³²Th, ^235,238U(n, γ), E ∼ 30 keV; analyzed available data; calculated s- and r-process abundances.

doi: 10.1093/mnras/stz3154
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2006DI21      Nucl.Phys. A777, 70 (2006)

R.Diehl, N.Prantzos, P.von Ballmoos

Astrophysical constraints from gamma-ray spectroscopy

doi: 10.1016/j.nuclphysa.2005.02.155
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2006RE07      Astrophys.J. 647, L41 (2006)

M.Renaud, J.Vink, A.Decourchelle, F.Lebrun, P.R.den Hartog, R.Terrier, C.Couvreur, J.Knodlseder, P.Martin, N.Prantzos, A.M.Bykov, H.Bloemen

The signature of ⁴⁴Ti in Cassiopeia a revealed by IBIS/ISGRI on INTEGRAL

doi: 10.1086/507300
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2005IS11      Nucl.Phys. A758, 603c (2005)

Y.Ishimaru, S.Wanajo, W.Aoki, S.G.Ryan, N.Prantzos

First enrichment of r-process elements in our Galaxy

doi: 10.1016/j.nuclphysa.2005.05.109
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2005PR17      Nucl.Phys. A758, 249c (2005)

N.Prantzos

The early phases of Milky Way's chemical evolution

doi: 10.1016/j.nuclphysa.2005.05.176
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2003HO19      Nucl.Phys. A718, 662c (2003)

J.L.Hou, N.Prantzos

Clues to the nucleosynthetic pattern and dust depletion in Damped Lyman α systems

doi: 10.1016/S0375-9474(03)00881-9
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2003IS14      Nucl.Phys. A718, 671c (2003)

Y.Ishimaru, N.Prantzos, S.Wanajo

Implications from Inhomogeneous Chemical Evolution: Yields of O-Zn

doi: 10.1016/S0375-9474(03)00884-4
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2003PR10      Nucl.Phys. A718, 309c (2003)

N.Prantzos

Perspectives in Galactic Chemical Evolution studies

doi: 10.1016/S0375-9474(03)00732-2
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2001HO20      Nucl.Phys. A688, 411c (2001)

J.L.Hou, N.Prantzos

Galactic Abundance Gradients and Implications for Nucleosynthesis

doi: 10.1016/S0375-9474(01)00740-0
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2001PR11      Nucl.Phys. A688, 37c (2001)

N.Prantzos, A.Goswami

Chemical Evolution of the Milky Way Halo and Disk

doi: 10.1016/S0375-9474(01)00664-9
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1999IL01      Astrophys.J. 524, 434 (1999)

C.Iliadis, P.M.Endt, N.Prantzos, W.J.Thompson

Explosive Hydrogen Burning of ²⁷Si, ³¹S, ³⁵Ar, and ³⁹Ca in Novae and X-Ray Bursts

NUCLEAR REACTIONS ²⁷Si, ³¹S, ³⁵Ar, ³⁹Ca(p, γ), E not given; calculated astrophysical reaction rates vs temperature.

doi: 10.1086/307778
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1997PR08      Nucl.Phys. A621, 558c (1997)

N.Prantzos

The Chemical Evolution of the Milky Way Disk

doi: 10.1016/S0375-9474(97)00303-5
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1994OL06      Astrophys.J. 424, 666 (1994)

K.A.Olive, N.Prantzos, S.Scully, E.Vangioni-Flam

Neutrino Process Nucleosynthesis and the ¹¹B/¹⁰B Ratio

doi: 10.1086/173922
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