利用 FAIR 的放射性离子进行核天体物理研究
天体物理仪器与方法
2016-01-13 v1 核实验
摘要
铁以外元素的核合成主要由 s 过程和 r 过程中的中子俘获主导。然而，32 种稳定的富质子同位素无法在这些过程中形成，因为它们被屏蔽在 s 过程流和 r 过程衰变链之外。这些原子核被认为源于 p 过程和 rp 过程。对于所有这些过程，当前的核天体物理研究致力于解决涉及放射性同位素的更精确反应数据的需求。根据特定反应的不同，研究人员通过正运动学或逆运动学、正向或时间反演方向进行调查，以确定或至少约束所需的反应截面。反质子与离子研究设施（FAIR）将为研究许多重要反应提供独特且前所未有的机会。其高产额的放射性同位素，即使远离稳定谷，也允许对涉及 r 过程或 rp 过程等奇异过程的同位素进行研究。
引用
@article{arxiv.1310.1632,
title = {Nuclear astrophysics with radioactive ions at FAIR},
author = {R. Reifarth and S. Altstadt and K. Göbel and T. Heftrich and M. Heil and A. Koloczek and C. Langer and R. Plag and M. Pohl and K. Sonnabend and M. Weigand and T. Adachi and F. Aksouh and J. Al-Khalili and M. AlGarawi and S. AlGhamdi and G. Alkhazov and N. Alkhomashi and H. Alvarez-Pol and R. Alvarez-Rodriguez and V. Andreev and B. Andrei and L. Atar and T. Aumann and V. Avdeichikov and C. Bacri and S. Bagchi and C. Barbieri and S. Beceiro and C. Beck and C. Beinrucker and G. Belier and D. Bemmerer and M. Bendel and J. Benlliure and G. Benzoni and R. Berjillos and D. Bertini and C. Bertulani and S. Bishop and N. Blasi and T. Bloch and Y. Blumenfeld and A. Bonaccorso and K. Boretzky and A. Botvina and A. Boudard and P. Boutachkov and I. Boztosun and A. Bracco and S. Brambilla and J. Briz Monago and M. Caamano and C. Caesar and F. Camera and E. Casarejos and W. Catford and J. Cederkall and B. Cederwall and M. Chartier and A. Chatillon and M. Cherciu and L. Chulkov and P. Coleman-Smith and D. Cortina-Gil and F. Crespi and R. Crespo and J. Cresswell and M. Csatlós and F. Déchery and B. Davids and T. Davinson and V. Derya and P. Detistov and P. Diaz Fernandez and D. DiJulio and S. Dmitry and D. Doré and J. Duenas and E. Dupont and P. Egelhof and I. Egorova and Z. Elekes and J. Enders and J. Endres and S. Ershov and O. Ershova and B. Fernandez-Dominguez and A. Fetisov and E. Fiori and A. Fomichev and M. Fonseca and L. Fraile and M. Freer and J. Friese and M. G. Borge and D. Galaviz Redondo and S. Gannon and U. Garg and I. Gasparic and L. Gasques and B. Gastineau and H. Geissel and R. Gernhäuser and T. Ghosh and M. Gilbert and J. Glorius and P. Golubev and A. Gorshkov and A. Gourishetty and L. Grigorenko and J. Gulyas and M. Haiduc and F. Hammache and M. Harakeh and M. Hass and M. Heine and A. Hennig and A. Henriques and R. Herzberg and M. Holl and A. Ignatov and A. Ignatyuk and S. Ilieva and M. Ivanov and N. Iwasa and B. Jakobsson and H. Johansson and B. Jonson and P. Joshi and A. Junghans and B. Jurado and G. Körner and N. Kalantar and R. Kanungo and A. Kelic-Heil and K. Kezzar and E. Khan and A. Khanzadeev and O. Kiselev and M. Kogimtzis and D. Körper and S. Kräckmann and T. Kröll and R. Krücken and A. Krasznahorkay and J. Kratz and D. Kresan and T. Krings and A. Krumbholz and S. Krupko and R. Kulessa and S. Kumar and N. Kurz and E. Kuzmin and M. Labiche and K. Langanke and I. Lazarus and T. Le Bleis and C. Lederer and A. Lemasson and R. Lemmon and V. Liberati and Y. Litvinov and B. Löher and J. Lopez Herraiz and G. Münzenberg and J. Machado and E. Maev and K. Mahata and D. Mancusi and J. Marganiec and M. Martinez Perez and V. Marusov and D. Mengoni and B. Million and V. Morcelle and O. Moreno and A. Movsesyan and E. Nacher and M. Najafi and T. Nakamura and F. Naqvi and E. Nikolski and T. Nilsson and C. Nociforo and P. Nolan and B. Novatsky and G. Nyman and A. Ornelas and R. Palit and S. Pandit and V. Panin and C. Paradela and V. Parkar and S. Paschalis and P. Pawłowski and A. Perea and J. Pereira and C. Petrache and M. Petri and S. Pickstone and N. Pietralla and S. Pietri and Y. Pivovarov and P. Potlog and A. Prokofiev and G. Rastrepina and T. Rauscher and G. Ribeiro and M. Ricciardi and A. Richter and C. Rigollet and K. Riisager and A. Rios and C. Ritter and T. Rodríguez Frutos and J. Rodriguez Vignote and M. Röder and C. Romig and D. Rossi and P. Roussel-Chomaz and P. Rout and S. Roy and P. Söderström and M. Saha Sarkar and S. Sakuta and M. Salsac and J. Sampson and J. Sanchez del Rio Saez and J. Sanchez Rosado and S. Sanjari and P. Sarriguren and A. Sauerwein and D. Savran and C. Scheidenberger and H. Scheit and S. Schmidt and C. Schmitt and L. Schnorrenberger and P. Schrock and R. Schwengner and D. Seddon and B. Sherrill and A. Shrivastava and S. Sidorchuk and J. Silva and H. Simon and E. Simpson and P. Singh and D. Slobodan and D. Sohler and M. Spieker and D. Stach and E. Stan and M. Stanoiu and S. Stepantsov and P. Stevenson and F. Strieder and L. Stuhl and T. Suda and K. Sümmerer and B. Streicher and J. Taieb and M. Takechi and I. Tanihata and J. Taylor and O. Tengblad and G. Ter-Akopian and S. Terashima and P. Teubig and R. Thies and M. Thoennessen and T. Thomas and J. Thornhill and G. Thungstrom and J. Timar and Y. Togano and U. Tomohiro and T. Tornyi and J. Tostevin and C. Townsley and W. Trautmann and T. Trivedi and S. Typel and E. Uberseder and J. Udias and T. Uesaka and L. Uvarov and Z. Vajta and P. Velho and V. Vikhrov and M. Volknandt and V. Volkov and P. von Neumann-Cosel and M. von Schmid and A. Wagner and F. Wamers and H. Weick and D. Wells and L. Westerberg and O. Wieland and M. Wiescher and C. Wimmer and K. Wimmer and J. S. Winfield and M. Winkel and P. Woods and R. Wyss and D. Yakorev and M. Yavor and J. Zamora Cardona and I. Zartova and T. Zerguerras and I. Zgura and A. Zhdanov and M. Zhukov and M. Zieblinski and A. Zilges and K. Zuber},
journal= {arXiv preprint arXiv:1310.1632},
year = {2016}
}
备注
Invited Talk given at the Conference Nuclear Physice in Astrophysics VI (NPA6), Lisbon, Portugal, May 19-24 2013. To appear in the NPA6 Proceedings in Journal of Physics: Conference Series (JPCS)