NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = L.Bildsten Found 5 matches. 2003SC24 Nucl.Phys. A718, 247c (2003) H.Schatz, L.Bildsten, A.Cumming, M.Ouellette Nuclear physics in normal X-ray bursts and superbursts
doi: 10.1016/S0375-9474(03)00722-X
2001SC21 Phys.Rev.Lett. 86, 3471 (2001) H.Schatz, A.Aprahamian, V.Barnard, L.Bildsten, A.Cumming, M.Ouellette, T.Rauscher, F.-K.Thielemann, M.Wiescher End Point of the rp Process on Accreting Neutron Stars NUCLEAR STRUCTURE Z=27-54; calculated astrophysical abundances; deduced rp-process endpoint.
doi: 10.1103/PhysRevLett.86.3471
2001SC29 Nucl.Phys. A688, 150c (2001) H.Schatz, A.Aprahamian, V.Barnard, L.Bildsten, A.Cumming, M.Ouellette, T.Rauscher, F.-K.Thielemann, M.Wiescher The Endpoint of the rp-Process on Accreting Neutron Stars
doi: 10.1016/S0375-9474(01)00688-1
1996ED02 Phys.Lett. 368B, 39 (1996); Erratum Phys.Lett. 380B, 493 (1996) C.M.Edwards, M.Palarczyk, D.Dehnhard, M.A.Espy, M.A.Franey, J.L.Langenbrunner, L.C.Bland, D.S.Carman, B.Brinkmoller, R.Madey, Y.Wang, J.W.Watson, L.Bildsten The 4He(p, n)4Li(*) Reaction at 100 and 200 MeV; Implications for the mass-four system and for astrophysics NUCLEAR REACTIONS 4He(p, nX), E=100, 200 MeV; measured inclusive σ(θ, En). 4Li deduced evidence for narrow states.
doi: 10.1016/0370-2693(95)01499-3
1990BI06 Nucl.Phys. A516, 77 (1990) L.Bildsten, I.Wasserman, E.E.Salpeter A Semi-Classical Model for Breakup Reactions of Light Nuclei: 4He(p, pn)3He NUCLEAR REACTIONS 4He(p, np), (p, 2p), E ≤ 300 MeV; calculated σ(E). Semi-classical model, breakup reactions.
doi: 10.1016/0375-9474(90)90050-V
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