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NSR database version of April 11, 2024.

Search: Author = A.Arcones

Found 19 matches.

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2022SC17      J.Phys.(London) G49, 110502 (2022)

H.Schatz, A.D.Becerril Reyes, A.Best, E.F.Brown, K.Chatziioannou, K.A.Chipps, C.M.Deibel, R.Ezzeddine, D.K.Galloway, C.J.Hansen, F.Herwig, A.P.Ji, M.Lugaro, Z.Meisel, D.Norman, J.S.Read, L.F.Roberts, A.Spyrou, I.Tews, F.X.Timmes, C.Travaglio, N.Vassh, C.Abia, P.Adsley, S.Agarwal, M.Aliotta, W.Aoki, A.Arcones, A.Aryan, A.Bandyopadhyay, A.Banu, D.W.Bardayan, J.Barnes, A.Bauswein, T.C.Beers, J.Bishop, T.Boztepe, B.Cote, M.E.Caplan, A.E.Champagne, J.A.Clark, M.Couder, A.Couture, S.E.de Mink, S.Debnath, R.J.deBoer, J.den Hartogh, P.Denissenkov, V.Dexheimer, I.Dillmann, J.E.Escher, M.A.Famiano, R.Farmer, R.Fisher, C.Frohlich, A.Frebel, C.Fryer, G.Fuller, A.K.Ganguly, S.Ghosh, B.K.Gibson, T.Gorda, K.N.Gourgouliatos, V.Graber, M.Gupta, W.C.Haxton, A.Heger, W.R.Hix, W.C.G.Ho, E.M.Holmbeck, A.A.Hood, S.Huth, G.Imbriani, R.G.Izzard, R.Jain, H.Jayatissa, Z.Johnston, T.Kajino, A.Kankainen, G.G.Kiss, A.Kwiatkowski, M.La Cognata, A.M.Laird, L.Lamia, P.Landry, E.Laplace, K.D.Launey, D.Leahy, G.Leckenby, A.Lennarz, B.Longfellow, A.E.Lovell, W.G.Lynch, S.M.Lyons, K.Maeda, E.Masha, C.Matei, J.Merc, B.Messer, F.Montes, A.Mukherjee, M.R.Mumpower, D.Neto, B.Nevins, W.G.Newton, L.Q.Nguyen, K.Nishikawa, N.Nishimura, F.M.Nunes, E.O'Connor, B.W.O'Shea, W.-J.Ong, S.D.Pain, M.A.Pajkos, M.Pignatari, R.G.Pizzone, V.M.Placco, T.Plewa, B.Pritychenko, A.Psaltis, D.Puentes, Y.-Z.Qian, D.Radice, D.Rapagnani, B.M.Rebeiro, R.Reifarth, A.L.Richard, N.Rijal, I.U.Roederer, J.S.Rojo, J.S K, Y.Saito, A.Schwenk, M.L.Sergi, R.S.Sidhu, A.Simon, T.Sivarani, A.Skuladottir, M.S.Smith, A.Spiridon, T.M.Sprouse, S.Starrfield, A.W.Steiner, F.Strieder, I.Sultana, R.Surman, T.Szucs, A.Tawfik, F.Thielemann, L.Trache, R.Trappitsch, M.B.Tsang, A.Tumino, S.Upadhyayula, J.O.Valle Martinez, M.Van der Swaelmen, C.Viscasillas Vazquez, A.Watts, B.Wehmeyer, M.Wiescher, C.Wrede, J.Yoon, R.G.T.Zegers, M.A.Zermane, M.Zingale, the Horizon 2020 Collaborations

Horizons: nuclear astrophysics in the 2020s and beyond

doi: https://dx.doi.org/10.1088/1361-6471/ac8890
Citations: PlumX Metrics


2021MO22      At.Data Nucl.Data Tables 142, 101453 (2021)

P.Mohr, Z.Fulop, Gy.Gyurky, G.G.Kiss, T.Szucs, A.Arcones, M.Jacobi, A.Psaltis

Astrophysical reaction rates of α-induced reactions for nuclei with 26 ≤ Z ≤ 83 from the new Atomki-V2 α-nucleus potential

NUCLEAR REACTIONS 88Kr, 188Sm(α, X), E(cm)<15 MeV; calculated astrophysical reaction rates using new Atomki-V2 α-nucleus potential and TALYS nuclear model code.

doi: 10.1016/j.adt.2021.101453
Citations: PlumX Metrics


2021SZ02      Phys.Rev. C 104, 035804 (2021)

T.N.Szegedi, G.G.Kiss, P.Mohr, A.Psaltis, M.Jacobi, G.G.Barnafoldi, T.Szucs, Gy.Gyurky, A.Arcones

Activation thick target yield measurement of 100Mo(α, n)103Ru for studying the weak r-process nucleosynthesis

NUCLEAR REACTIONS 100Mo(α, n)103Ru, E=7.0-13.0 MeV; measured Eγ, Iγ, thick target σ(E) by activation technique at the Institute for Nuclear Research (Atomki); deduced recommended astrophysical rate at T9=1.0-5.0, elemental abundances for the MC13 trajectory using α-nucleus optical model potentials (α-OMPs) with Atomki-V2 potential to model the nucleosynthesis scenario. 95,97Ru, 95Tc; observed γ rays in the spectrum.

doi: 10.1103/PhysRevC.104.035804
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4422.


2020BL01      Phys.Rev. C 101, 055807 (2020)

J.Bliss, A.Arcones, F.Montes, J.Pereira

Nuclear physics uncertainties in neutrino-driven, neutron-rich supernova ejecta

NUCLEAR REACTIONS 59,68Fe, 63,71Co, 74,76Ni, 67,77Cu, 72,76,78,79,80Zn, 81Ga, 78,80,82Ge, 83As, 84,85Se, 85,87,88Br, 86,87,88,89,90Kr, 87,89Rb, 88,89,90,91,92,93,94Sr, 94,95Y, 94,95,96,97,98Zr, 97Nb(α, n), T=1-5 GK; calculated abundances of lighter heavy elements with a reaction network under different astrophysical conditions, by varying (α, n) reaction rates within their theoretical uncertainties using a Monte Carlo approach; deduced Spearman's correlation coefficients for Z=36-47, and most important (α, n) reactions affecting the nucleosynthesis in core-collapse supernovae (CCSNe).

doi: 10.1103/PhysRevC.101.055807
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2020YA05      Phys.Rev.Lett. 124, 092701 (2020)

H.Yasin, S.Schafer, A.Arcones, A.Schwenk

Equation of State Effects in Core-Collapse Supernovae

doi: 10.1103/PhysRevLett.124.092701
Citations: PlumX Metrics


2020YA07      Phys.Rev.Lett. 124, 092701 (2020)

H.Yasin, S.Schafer, A.Arcones, A.Schwenk

Equation of State Effects in Core-Collapse Supernovae

doi: 10.1103/PhysRevLett.124.092701
Citations: PlumX Metrics


2019HO18      J.Phys.(London) G46, 083001 (2019)

C.J.Horowitz, A.Arcones, B.Cote, I.Dillmann, W.Nazarewicz, I.U.Roederer, H.Schatz, A.Aprahamian, D.Atanasov, A.Bauswein, T.C.Beers, J.Bliss, M.Brodeur, J.A.Clark, A.Frebel, F.Foucart, C.J.Hansen, O.Just, A.Kankainen, G.C.McLaughlin, J.M.Kelly, S.N.Liddick, D.M.Lee, J.Lippuner, D.Martin, J.Mendoza-Temis, B.D.Metzger, M.R.Mumpower, G.Perdikakis, J.Pereira, B.W.O'Shea, R.Reifarth, A.M.Rogers, D.M.Siegel, A.Spyrou, R.Surman, X.Tang, T.Uesaka, M.Wang

r-process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos

doi: 10.1088/1361-6471/ab0849
Citations: PlumX Metrics


2017AR04      Prog.Part.Nucl.Phys. 94, 1 (2017)

A.Arcones, D.W.Bardayan, T.C.Beers, L.A.Bernstein, J.C.Blackmon, B.Messer, B.A.Brown, E.F.Brown, C.R.Brune, A.E.Champagne, A.Chieffi, A.J.Couture, P.Danielewicz, R.Diehl, M.El Eid, J.E.Escher, B.D.Fields, C.Frohlich, F.Herwig, W.R.Hix, C.Iliadis, W.G.Lynch, G.C.McLaughlin, B.S.Meyer, A.Mezzacappa, F.Nunes, B.W.O'Shea, M.Prakash, B.Pritychenko, S.Reddy, E.Rehm, G.Rogachev, R.E.Rutledge, H.Schatz, M.S.Smith, I.H.Stairs, A.W.Steiner, T.E.Strohmayer, F.X.Timmes, D.M.Townsley, M.Wiescher, R.G.T.Zegers, M.Zingale

White paper on nuclear astrophysics and low energy nuclear physics Part 1: Nuclear astrophysics

doi: 10.1016/j.ppnp.2016.12.003
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2017BL03      J.Phys.(London) G44, 054003 (2017)

J.Bliss, A.Arcones, F.Montes, J.Pereira

Impact of (α, n) reactions on weak r-process in neutrino-driven winds

NUCLEAR REACTIONS 69Ga, 100Mo(α, n), (α, 2n), E(cm)<24 MeV; calculated yields, abundances using TALYS 1.6 nuclear reaction code. Comparison with available data.

doi: 10.1088/1361-6471/aa63bd
Citations: PlumX Metrics


2016CA25      Phys.Rev.Lett. 117, 012501 (2016)

R.Caballero-Folch, C.Domingo-Pardo, J.Agramunt, A.Algora, F.Ameil, A.Arcones, Y.Ayyad, J.Benlliure, I.N.Borzov, M.Bowry, F.Calvino, D.Cano-Ott, G.Cortes, T.Davinson, I.Dillmann, A.Estrade, A.Evdokimov, T.Faestermann, F.Farinon, D.Galaviz, A.R.Garcia, H.Geissel, W.Gelletly, R.Gernhauser, M.B.Gomez Hornillos, C.Guerrero, M.Heil, C.Hinke, R.Knobel, I.Kojouharov, J.Kurcewicz, N.Kurz, Yu.A.Litvinov, L.Maier, J.Marganiec, T.Marketin, M.Marta, T.Martinez, G.Martinez-Pinedo, F.Montes, I.Mukha, D.R.Napoli, C.Nociforo, C.Paradela, S.Pietri, Zs.Podolyak, A.Prochazka, S.Rice, A.Riego, B.Rubio, H.Schaffner, Ch.Scheidenberger, K.Smith, E.Sokol, K.Steiger, B.Sun, J.L.Tain, M.Takechi, D.Testov, H.Weick, E.Wilson, J.S.Winfield, R.Wood, P.Woods, A.Yeremin

First Measurement of Several β-Delayed Neutron Emitting Isotopes Beyond N = 126

RADIOACTIVITY 204,205,206Au, 208,209,210,211Hg, 211,212,213Tl, 214,215,216Tl, 215,216,217,218Pb, 218,219,220Bi(β-n) [from Be(238U, X), E=1 GeV/nucleon]; measured decay products, Eβ, Iβ, En, In, β-n coinc.; deduced T1/2, neutron branching ratios. Comparison with available data, theoretical calculations.

doi: 10.1103/PhysRevLett.117.012501
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23395. Data from this article have been entered in the XUNDL database. For more information, click here.


2016MA22      Phys.Rev.Lett. 116, 121101 (2016)

D.Martin, A.Arcones, W.Nazarewicz, E.Olsen

Impact of Nuclear Mass Uncertainties on the r Process

NUCLEAR STRUCTURE A=80-240; calculated isotopic abundances for neutron star and supernovae, two-neutron separation energies using SkM, SLy4, and UNEDF0 models.

doi: 10.1103/PhysRevLett.116.121101
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2014AR01      J.Phys.(London) G41, 044005 (2014)

A.Arcones, J.Bliss

Nucleosynthesis of elements between Sr and Ag in neutron- and proton-rich neutrino-driven winds

doi: 10.1088/0954-3899/41/4/044005
Citations: PlumX Metrics


2012AR09      J.Phys.:Conf.Ser. 337, 012041 (2012)

A.Arcones

"Heavy" elements produced in neutrino-driven winds

doi: 10.1088/1742-6596/337/1/012041
Citations: PlumX Metrics


2011AR04      Phys.Rev. C 83, 045809 (2011)

A.Arcones, G.Martinez-Pinedo

Dynamical r-process studies within the neutrino-driven wind scenario and its sensitivity to the nuclear physics input

doi: 10.1103/PhysRevC.83.045809
Citations: PlumX Metrics


2011AR20      J.Phys.:Conf.Ser. 312, 042005 (2011)

A.Arcones

Explosive nucleosynthesis in core-collapse supernovae

doi: 10.1088/1742-6596/312/4/042005
Citations: PlumX Metrics


2011TH01      Prog.Part.Nucl.Phys. 66, 346 (2011)

F.-K.Thielemann, A.Arcones, R.Kappeli, M.Liebendorfer, T.Rauscher, C.Winteler, C.Frohlich, I.Dillmann, T.Fischer, G.Martinez-Pinedo, K.Langanke, K.Farouqi, K.-L.Kratz, I.Panov, I.K.Korneev

What are the astrophysical sites for the r-process and the production of heavy elements?

doi: 10.1016/j.ppnp.2011.01.032
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2010AR08      J.Phys.:Conf.Ser. 202, 012007 (2010)

A.Arcones, G.Martinez-Pinedo

Nucleosynthesis in neutrino-driven winds: Influence of the nuclear physics input

doi: 10.1088/1742-6596/202/1/012007
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2010PE18      J.Phys.:Conf.Ser. 202, 012008 (2010)

I.Petermann, G.Martinez-Pinedo, A.Arcones, W.R.Hix, A.Kelic, K.Langanke, I.Panov, T.Rauscher, K.-H.Schmidt, F.-K.Thielemann, N.Zinner

Network calculations for r-process nucleosynthesis

doi: 10.1088/1742-6596/202/1/012008
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2008AR06      Phys.Rev. C 78, 015806 (2008)

A.Arcones, G.Martinez-Pinedo, E.O'Connor, A.Schwenk, H.-Th.Janka, C.J.Horowitz, K.Langanke

Influence of light nuclei on neutrino-driven supernova outflows

NUCLEAR REACTIONS 3H(ν-bar, ν-bar), (ν-bar, e+), E=11-100 MeV; calculated σ.

doi: 10.1103/PhysRevC.78.015806
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