Importancia de la línea de goteo de los protones de los núcleos para la astrofísica nuclear

Contenido principal del artículo

Lídia S. Ferreira
Enrico Maglione

Resumen

Discutimos los resultados recientes sobre la desintegración de los núcleos exóticos ricos en protones en la línea de goteo de protones con Z <50, que son de gran importancia para los modelos de astrofísica nuclear.

Detalles del artículo

Cómo citar
Ferreira, L. S., & Maglione, E. (2019). Importancia de la línea de goteo de los protones de los núcleos para la astrofísica nuclear. Nucleus, (63), 58-61. Recuperado a partir de http://nucleus.cubaenergia.cu/index.php/nucleus/article/view/649
Sección
Ciencias Nucleares

Citas

[1] THOENNESSEN M & SHERRILL BM. From isotopes to the stars. Nature. 2011; 473(7345): 25-26.
[2] SONZOGNI AA. Proton Radioactivity in Z > 50 Nuclides. Nucl. Data Sheets 2002; 95(1): 1-48.
[3] BLANK B & PLOSZAJCZAK M. Two-proton radioactivity. Rep. Prog. Phys. 2008; 71(4): 046301.
[4] BLANK B & BORGE M. Nuclear structure at the proton drip line: Advances with nuclear decay studies. Prog. Part. and Nucl. Phys. 2008; 60(2): 403-483.
[5] ARNOULD M & GORIELY S. The p-process of stellar nucleosynthesis: astrophysics and nuclear physics status. Phys. Rep. 2003; 384(1-2): 1.
[6] SCHATZ H & REHM KE. X-ray binaries. Nucl. Phys. A. 2006; 777: 601-622.
[7] SCHATZ H, APRAHAMIAN A, BARNARD V, et. al. End point of the rp process on accreting neutron stars. Phys. Rev. Lett. 2001; 86(16): 3471.
[8] WOODS PJ & DAVIDS CN. Nuclei beyond the proton drip-line. Ann. Rev. Nucl. and Part. Science. 1997; 47(): 541-590.
[9] PROCTER MG, et. al. Proton emission from an oblate nucleus 151Lu. Phys. Lett. B. 2013; 725(1-3): 79-84.
[10] FIORIN G, MAGLIONE E & FERREIRA LS. Theoretical description of deformed proton emitters: nonadiabatic quasiparticle method. Phys. Rev. C. 2003; 67(5): 054302.
[11] TAYLOR MJ, et. al. Oblately deformed isomeric proton-emitting state in 151Lu. Phys. Rev. C. 2015; 91(4): 044322.
[12] PATIAL M, ARUMUGAM P, JAIN AK, et. al. Nonadiabatic quasiparticle approach for deformed odd-odd nuclei and the proton emitter 130Eu. Phys. Rev. C. 2013; 88(5): 054302.
[13] MODI S, PATIAL M , ARUMUGAM P , et. al. Triaxiality in the proton emitter 109I. Phys. Rev. C. 2017; 95(5): 054323.
[14] ALMARAZ-CALDERON S, et. al. Level structure of 18Ne and its importance in the 14O(?,p)17F reaction rate. Phys. Rev. C. 2012; 86(2): 025801.
[15] RACITI G, et. al. Experimental Evidence of 2He Decay from 18Ne Excited States Phys. Rev. Lett. 2008; 100(19): 192503.
[16] LIN CJ, et. al. Recent experimental results of two?proton correlated emission from the excited states of 17,18Ne and 28,29S. AIP Conf. Proc. 2011; 98: 1409.

[17] BROWN BA, BARKER FC & MILLENER DJ. Phys. Rev. C. 2002; 65(): 051309(R).
[18] BOUHELAL M, et. al. Nuc. Phys. A. 2011; 864(): 113.
[19] SUZUKI H, SÖDERSTRÖM PA, LORUSSO G, et. al. Discovery of 72Rb: a nuclear sandbank beyond the proton drip line. Phys. Rev. Lett. 2017; 119(19): 192503.
[20] MOLLER P, NIX JR, & KRATZ KL. At. Data Nucl. Data Tab. 1997; 66(): 131.
[21] HUANG W, AUDI G, WANG M, et. al. The AME2016 atomic mass evaluation (I). Evaluation of input data; and adjustment procedures. Chin. Phys. C. 2017; 41(3): 030002.
[22] WANG M , AUDI G , KONDEV F, et. al. The AME2016 atomic mass evaluation (II). Tables, graphs and references. Chin. Phys. C. 2017; 41(3): 030003.
[23] SINCLAIR L. Ph.D. thesis. University of York. 2016.
[23] FERREIRA LS & MAGLIONE E. Odd-Odd Deformed Proton Emitters. Phys. Rev. Lett. 2001; 86(9): 1721.