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58. Assessing the cardiology community position on transradial intervention and the use of bivalirudin in patients with acute coronary syndrome undergoing invasive management: results of an EAPCI survey

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Adamo, Marianna, Byrne, Robert A., Baumbach, Andreas, Haude, Michael, Windecker, Stephan, Valgimigli, Marco, Aaroe, J., Abdeltawab, A. A., Accardi, R., Addad, F., Agostoni, P., Alajab, A., Alcázar, E., Alhabil, B., Altug Cakmak, H., Amico, F., Amoroso, G., Anderson, R., Andò, G., Andreou, A. Y., Antoniadis, D., Aquilina, M., Aramberry, L., Auer, J., Auffret, V., Ausiello, A., Austin, D., Avram, A., Ayman, E., Babunashvili, V., Bagur, R., Bakotic, Z., Balducelli, M., Ballesteros, S. M., Baptista, S., Baranauskas, A., Barbeau, G., Bax, M., Benchimol, C., Berroth, R., Biasco, L., Bilal, A., Binias, K., Blanco Mata, R., Boccuzzi, G., Bolognese, L., Boskovic, S., Bourboulis, N., Briguori, C., Bunc, M., Buysschaert, I., Calabro’, P., Campo, G., Candiello, A., Caprotta, U. F., Cardenas, M., Carrilho-Ferreira, P., Carrizo, S., Caruso, M., Cassar, A., Cernigliaro, C., Chacko, G., Chamie, D., Clapp, B., Coceani, M., Colangelo, S., Colombo, A., Comeglio, M., Connaughton, M., Conway, D., Cortese, B., Cosgrave, J., Costa, F., Couvoussis, E., Crimi, G., Crook, R., Cruz-Alvarado, J. E., Curello, S., D’Ascenzo, F., D’Urbano, M., Dana, A., De Backer, O., De Carlo, M., De Cesare, N., De Iaco, G., De La Torre, H. J. M., De Oliveira Netoj, B., Devlin, G. P., Di Lorenzo, E., Díaz, A., Dina, C., Dorsel, T. H., Eberli, F. R., Echeverría, R., Eftychiou, C., Elguindy, A., Ercilla, J., Ernst, A., Esposito, G., Ettori, F., Eufracino, Null, Ezquerra Aguilera, W., Falcone, C., Falu, R. M., Feres, F., Ferlini, M., Fernández, G., Fernández-Rodríguez, D., Fileti, L., Fischetti, D., Florescu, N., Formigli, D., Fouladvand, F., Franco, N., Fresco, C., Frigoli, E., Furmaniuk, J., Gabaldo, K., Galli, M., Galli, S., Garbo, R., Garducci, S., Garg, S., Gavrielatos, G., Gensch, J., Giacchi, G., Giunio, L., Giustino, G., Goldberg, L., Goldsmit, R., Gommeaux, A., González Godínez, H., Gosselin, G., Govorov, A., Grimfjard, P., Gross, E., Grosz, C., Guagliumi, G., Hadad, W., Hadadi, L., Hansen, P. R., Harb, S., Hatrick, R., Hayrapetyan, H. G., Hernández-Enríquez, M., Ho Heo, J., Horvath, I. G., Huan Loh, P., Ibrahim, A. M., Ierna, S., Ilic, I., Imperadore, F., Ionescu-Silva, E., Jacksch, R., James, S., Janiak, B., Jensen, S. E., Jeroen, S., Jugessur, R. K., Kala, P., Kambis, M., Kanakakis, J., Karamasis, G., Karchevsky, D., Karpovskiy, A., Kayaert, P., Kedev, S., Kemala, E., Ketteler, T., Khan, S. Q., Kharlamov, A., Kiernan, T., Kiviniem, T., Koltowski, L., Koskinas, K. C., Kouloumpinis, A., Kraaijeveld, A. O., Krizanic, F., Krötz, B., Kuczmik, W., Kukreja, N., Kuksa, D., Yav, K., Kyriakos, D., Labrunie, A., Laine, M., Lapin, O., Larosa, C., Latib, A., Lattuca, B., Lauer, B., Lefèvre, T., Legrand, V., Lehto, P., Leiva-Pons, J. L., Leone, A. M., Lev, G., Lim, R., Limbruno, U., Linares Vicente, J. A., Lindsay, S., Linnartz, C., Liso, A., Lluberas, R., Locuratolo, N., Lokshyn, S., Lunde, K., Lupi, A., Magnavacchi, P., Maia, F., Mainar, V., Mancone, M., Manolios, M. G., Mansour, S., Mariano, E., Marques, K., Martins, H., Mckenzie, D., Meco, S., Meemook, K., Mehmed, K., Melikyan, A., Mellwig, K. P., Mendiz, O. A., Merkulov, E., Mesquita, H. G., Mezzapelle, G., Miloradovic, V., Mohamed, S., Mohammed, B., Mohammed, F., Mohammed, K., Mohanad, A., Morawiec, B., More, R., Moreno-Martínez, F. L., Mrevlje, B., Muhammad, F., Näveri, H., Nazzaro, M. S., Neary, P., Negus, B. H., Nelson Durval, F. G., Nick, H., Nilva, E., Oldroyd, K. G., Olivares Asencio, C., Omerovic, E., Ortiz, M. A., Ota, H., Otasevic, P., Otieno, H. A., Paizis, I., Papp, E., Pasquetto, G., Patsourakos, N. G., Peels, J., Pelliccia, F., Pennacchi, M., Penzo, C., Perez, P., Perkan, A., Petrou, E., Phipathananunth, W., Pierri, A., Pinheiro, L. F., Pipa, J. L., Piva, T., Polad, J., Porto, I., Poveda, J., Predescu, L., Prog, R., Puri, R., Raco, D. L., Ramazan, O., Ramazzotti, V., Rao, S. V., Raungaard, B., Reczuch, K., Rekik, S., Rhouati, A., Rigattieri, S., Rodríguez-Olivares, R., Roik, M., Romagnoli, E., Román, A. J., Routledge, H., Rubartelli, P., Rubboli, A., Ruiz-García, J., Russo, F., Ruzsa, Z., Ryding, A., Saad, Aly, Sabate, M., Sabouret, P., Sadowski, M., Saia, F., Sanchez Perez, I., Santoro, G. M., Sarenac, D., Saririan, M., Sarma, J., Schuetz, T., Sciahbasi, A., Sebastian, M., Sebik, R., Sesana, M., Hur, Seung-Ho, Sganzerla, P., Shalva, R., Sharma, S., Sheiban, I., Shein, K. K., Shiekh, I. A., Sinha, M., Slhessarenko, J., Smith, D., Smyth, D. W., Sönmez, K., Sood, N., Sourgounis, A., Srdanovic, I., Stables, R. H., Stefanini, G. G., Stewart, J., Stoyanov, N., Suliman, A. A., Suryadevara, R., Suwannasom, P., Tange Veien, K., Tauchert, S., Tebet, M., Testa, L., Thury, A., Tilsted, H. H., Tiroch, K., Torres, A., Tosi, P., Traboulsi, M., Trani, C., Tresoldi, S., Tsigkas, G., Tueller, D., Turri, M., Udovichenko, A. E., Uretsky, B., Van Der Harst, P., Van Houwelingen, K. G., Vandoni, P., Vandormael, M., Varbella, F., Venkitachalam, C. G., Vercellino, M., Vidal-Perez, R., Vigna, C., Vignali, L., Vogt, F., Voudris, V., Vranckx, P., Vrolix, M., Vydt, T., Webster, M., Wijns, W., Woody, W., Wykrzykowska, J., Yazdani, S., Yildiz, A., Yurlevich, D., Zauith, R., Zekanovic, D., Zhao, M., Zimarino, M., Zingarelli, A., Abdelsamad, A. Y., Abo Shaera, E. S., Afshar, M. S., Agatiello, C., Aguiar, P., Ahmad, A. M., Akin, I., Alameda, M., Alegría-Barrero, E., Alejos, R., Alkhashab, K., Alkutshan, R. S. A., Almorraweh, A., Altnji, I., Alvarez Iorio, C., Anchidin, O., Angel, J., Antonopoulos, A., Apshilava, G., Arana, C., Ashikaga, T., Assomull, R., Atef, S. Z., Azmus, A. D., Azzalini, L., Azzouz, A., Baglioni, P., Bampas, G., Basil, M. P., Baumbach, A., Besh, D., Bhushan Sharm, A., Bien Hsien, H., Bihui, L., Bing-Chen, L., Biryukov, S., Blatt, A., Bocchi, E., Boghdady, A., Bonarjee, V. V. S., Bosnjak, I., Bravo Baptista, S., Brinckman, S. L., Buchter, B., Burzotta, F., Cacucci, M., Cagliyan, C. E., Calabrò, P., Cernetti, C., Chávez Mizraym, R., Choo, W. S., Choudhury, R., Cicco, N., Cisneros Clavijo, P., Çitaku, H., Collet, J. P., Consuegra-Sánchez, L., Conte, M., Corral, J. M., Damonte, A., Dangoisse, V., Dastani, M., Della Rosa, F., Deora, S., Devadathan, S., Dharma, S., Di Giorgio, A., Diez, J. L., Dinesha, B., Duplančić, D., El Behwashi, M. F., Elghawaby, H., Elshahawy, O., Eskola, M. J., Etman, A., Eun Gyu, L., Fabiano, L., Facta, A., Fan, Y., Fang-Yang, H., Farag, E., Fathi, Y., Fazeli, N., Federico, P., Fereidoun, M. Z., Fernandez-Nofrerias, E., Flensted Lassen, J., Flessas, D., Fouad, H., Franco-Pelaez, J. A., Fu, Q., Furtado, R., Gadepalli, R., Gallino, R., Gasparetto, V., Gentiletti, A., Gholoobi, A., Ghosh, A. K., Gkizas, S., Golchha, S. K., Goncharov, A., Gössl, M., Götberg, M., Greco, F., Grundeken, M. J., Gupta, D., Gupta, S., Guray, U., Hahalis, G., Hakim Vista, J., Hamid, M. A., Hammoudeh, A., Hasan, A. R. I., Hatsumura, F. E., Heintzen, M. P., Helal, T., Hetherington, S., Hewarathna, U. I., Hioki, H., Hissein, F., Ho-Ping, Y., Homs, S., Huber, K., Ibarra, F. M., Ielasi, A., Ipek, E., Jambunathan, R., Jamshidi, P., Jarrad, I., Javier, W., Jensen, J., Jimenez-Quevedo, P., Kalpak, O., Kan, J., Kanaan, T., Kao, D. H. M., Karamfiloff, K., Karegren, A., Karjalainen, P. P., Kasabov, R., Katsimagklis, G. D., Kaul, U., Khan, A., Kiemeneij, E., Kiviniemi, T., Kleiban, A., Komiyama, N., Konteva, M., Koshy, G., Krepsky, A. M., Kuljit, S., Kulkarni, P., Kumar, V., Kuznetsov, I., Lai, G., Lateef, M. A., Lawand, S., Le Hong, T., Lettieri, C., Levy, G., Lindvall, P., Maitra, A., Makowski, M., Mamas, M. A., Mandal, S. C., Mangalanandan, P., Marin, R., Mashhadi, M., Matsukage, T., Meier, B., Milosavljevic, B., Miro, S. S., Mitov, A., Moeriel, M., Moguel, R., Mohanty, A., Montalescot, G., Mörsdorf, W., Moscato, F., Muniz, A., Muraglia, S., Myć, J., Nada, A., Nair, P., Namazi, M. H., Naraghipour, F., Nguyen, Q. N., Nicosia, A., Nikas, D., Ober, M., Ocaranza-Sánchez, R., Olivecrona, G., Pahlajani, D., Pandey, B. P., Parma, A., Parma, R., Patsilinakos, S. P., Pattam, J., Peddi, S., Perez, P. R., Peruga, J. Z., Pescoller, F., Petrov, I., Piatti, L., Pico-Aracil, F., Pina, J., Piroth, Z., Popa, V., Pourbehi, M. R., Pradhan, A. K., Prida, X. E., Purohit, B. V., Pyun, W. B., Quang Hung, D., Rada, I., Rafizadeh, O., Rahman, M. A., Rai, L., Ramsewak, A., Ravindran, R., Rodriguez De Leiras, O. S., Rodríguez Esteban, M., Roque Figueira, H., Saket, A., Sakhov, O., Saktheeswaran, M. K., Salachas, A., Sallam, A., Sampaolesi, A., Samy, A., Sanchis, J., Santaera, O., Santarelli, A., Santharaj, W. S., Sarango, B., Satheesh, S., Schmitz, T., Schühlen, H., Seewoosagur, R., Segev, A., Seisembekov, V., Semitko, S., Sengottuvelu, G., Sepulveda Varela, P., Sethi, A., Sharma, A., Sharma, R. K., Shi, Hy., Şimşek, M. A., Siqueira, B., Skalidis, E., Slawin, J., Sorokhtey, L., Spaulding, C., Srinivas, B., Srinivasan, M., Stakos, D., Stefanini, G., Stojkovic, S., Tacoy, G., Tawade, M., Tiecco, F., Tondi, S., Torresani, E. M., Tousek, P., Tran, T., Trantalis, G., Triantafyllou, K., Trivedi, R., Trivisonno, A., Tsui, K. L., Türkoğlu, C., Tzung-Dau, W., Ueno, H., Urban, U., Uretsky, B. F., Uscumlic, A., Venugopal, V., Verney, R., Vilar, J. V., Villacorta, V. G., Vishwanath, R., Vlachojannis, G. J., Vlachojannis, M., Vlad, V., Von Birgelen, C., Vukcevic, V., Wahab, A., Waksman, R., Wei-Wen, L., Weisz, G., Whittaker, A., Yadav, A., Yokoi, Y., Zacharoulis, A., Zahran, M., Zamani, J., Ziakas, A., Zimmermann, J. P., Adamo, M., Byrne, R. A., Baumbach, A., Haude, M., Windecker, S., Valgimigli, M., Aaroe, J., Abdeltawab, A. A., Accardi, R., Addad, F., Agostoni, P., Alajab, A., Alcazar, E., Alhabil, B., Altug Cakmak, H., Amico, F., Amoroso, G., Anderson, R., Ando, G., Andreou, A. Y., Antoniadis, D., Aquilina, M., Aramberry, L., Auer, J., Auffret, V., Ausiello, A., Austin, D., Avram, A., Ayman, E., Babunashvili, V., Bagur, R., Bakotic, Z., Balducelli, M., Ballesteros, S. M., Baptista, S., Baranauskas, A., Barbeau, G., Bax, M., Benchimol, C., Berroth, R., Biasco, L., Bilal, A., Binias, K., Blanco Mata, R., Boccuzzi, G., Bolognese, L., Boskovic, S., Bourboulis, N., Briguori, C., Bunc, M., Buysschaert, I., Calabro', P., Campo, G., Candiello, A., Caprotta, U. F., Cardenas, M., Carrilho-Ferreira, P., Carrizo, S., Caruso, M., Cassar, A., Cernigliaro, C., Chacko, G., Chamie, D., Clapp, B., Coceani, M., Colangelo, S., Colombo, A., Comeglio, M., Connaughton, M., Conway, D., Cortese, B., Cosgrave, J., Costa, F., Couvoussis, E., Crimi, G., Crook, R., Cruz-Alvarado, J. E., Curello, S., D'Ascenzo, F., D'Urbano, M., Dana, A., De Backer, O., De Carlo, M., De Cesare, N., De Iaco, G., De La Torre, H. J. M., De Oliveira Netoj, B., Devlin, G. P., Di Lorenzo, E., Diaz, A., Dina, C., Dorsel, T. H., Eberli, F. R., Echeverria, R., Eftychiou, C., Elguindy, A., Ercilla, J., Ernst, A., Esposito, G., Ettori, F., Eufracino, Ezquerra Aguilera, W., Falcone, C., Falu, R. M., Feres, F., Ferlini, M., Fernandez, G., Fernandez-Rodriguez, D., Fileti, L., Fischetti, D., Florescu, N., Formigli, D., Fouladvand, F., Franco, N., Fresco, C., Frigoli, E., Furmaniuk, J., Gabaldo, K., Galli, M., Galli, S., Garbo, R., Garducci, S., Garg, S., Gavrielatos, G., Gensch, J., Giacchi, G., Giunio, L., Giustino, G., Goldberg, L., Goldsmit, R., Gommeaux, A., Gosselin, G., Govorov, A., Gonzalez Godinez, H., Gross, E., Grosz, C., Guagliumi, G., Hadad, W., Hadadi, L., Hansen, P. R., Harb, S., Hatrick, R., Hayrapetyan, H. G., Hernandez-Enriquez, M., Ho Heo, J., Horvath, I. G., Huan Loh, P., Ibrahim, A. M., Ierna, S., Ilic, I., Imperadore, F., Ionescu-Silva, E., Jacksch, R., James, S., Janiak, B., Jensen, S. E., Jeroen, S., Jugessur, R. K., Kala, P., Kambis, M., Kanakakis, J., Karamasis, G., Karchevsky, D., Karpovskiy, A., Kayaert, P., Kedev, S., Kemala, E., Ketteler, T., Khan, S. Q., Kharlamov, A., Kiernan, T., Kiviniem, T., Koltowski, L., Koskinas, K. C., Kouloumpinis, A., Kraaijeveld, A. O., Krizanic, F., Krotz, B., Kuczmik, W., Kukreja, N., Kuksa, D., Yav, K., Kyriakos, D., Labrunie, A., Laine, M., Lapin, O., Larosa, C., Latib, A., Lattuca, B., Lauer, B., Lefevre, T., Legrand, V., Lehto, P., Leiva-Pons, J. L., Leone, A. M., Lev, G., Lim, R., Limbruno, U., Linares Vicente, J. A., Lindsay, S., Linnartz, C., Liso, A., Lluberas, R., Locuratolo, N., Lokshyn, S., Lunde, K., Lupi, A., Magnavacchi, P., Maia, F., Mainar, V., Mancone, M., Manolios, M. G., Mansour, S., Mariano, E., Marques, K., Martins, H., Mckenzie, D., Meco, S., Meemook, K., Mehmed, K., Melikyan, A., Mellwig, K. P., Mendiz, O. A., Merkulov, E., Mesquita, H. G., Mezzapelle, G., Miloradovic, V., Mohamed, S., Mohammed, B., Mohammed, F., Mohammed, K., Mohanad, A., Morawiec, B., More, R., Moreno-Martinez, F. L., Mrevlje, B., Muhammad, F., Naveri, H., Nazzaro, M. S., Neary, P., Negus, B. H., Nelson Durval, F. G., Nick, H., Nilva, E., Oldroyd, K. G., Olivares Asencio, C., Omerovic, E., Ortiz, M. A., Ota, H., Otasevic, P., Otieno, H. A., Paizis, I., Papp, E., Pasquetto, G., Patsourakos, N. G., Peels, J., Pelliccia, F., Pennacchi, M., Penzo, C., Perez, P., Perkan, A., Petrou, E., Phipathananunth, W., Pierri, A., Pinheiro, L. F., Pipa, J. L., Piva, T., Polad, J., Porto, I., Poveda, J., Predescu, L., Prog, R., Puri, R., Raco, D. L., Ramazan, O., Ramazzotti, V., Rao, S. V., Raungaard, B., Reczuch, K., Rekik, S., Rhouati, A., Rigattieri, S., Rodriguez-Olivares, R., Roik, M., Romagnoli, E., Roman, A. J., Routledge, H., Rubartelli, P., Rubboli, A., Ruiz-Garcia, J., Russo, F., Ruzsa, Z., Ryding, A., Saad, A., Sabate, M., Sabouret, P., Sadowski, M., Saia, F., Sanchez Perez, I., Santoro, G. M., Sarenac, D., Saririan, M., Sarma, J., Schuetz, T., Sciahbasi, A., Sebastian, M., Sebik, R., Sesana, M., Hur, S. -H., Sganzerla, P., Shalva, R., Sharma, S., Sheiban, I., Shein, K. K., Shiekh, I. A., Sinha, M., Slhessarenko, J., Smith, D., Smyth, D. W., Sonmez, K., Sood, N., Sourgounis, A., Srdanovic, I., Stables, R. H., Stefanini, G. G., Stewart, J., Stoyanov, N., Suliman, A. A., Suryadevara, R., Suwannasom, P., Tange Veien, K., Tauchert, S., Tebet, M., Testa, L., Thury, A., Tilsted, H. H., Tiroch, K., Torres, A., Tosi, P., Traboulsi, M., Trani, C., Tresoldi, S., Tsigkas, G., Tueller, D., Turri, M., Udovichenko, A. E., Uretsky, B., Van Der Harst, P., Van Houwelingen, K. G., Vandoni, P., Vandormael, M., Varbella, F., Venkitachalam, C. G., Vercellino, M., Vidal-Perez, R., Vigna, C., Vignali, L., Vogt, F., Voudris, V., Vranckx, P., Vrolix, M., Vydt, T., Webster, M., Wijns, W., Woody, W., Wykrzykowska, J., Yazdani, S., Yildiz, A., Yurlevich, D., Zauith, R., Zekanovic, D., Zhao, M., Zimarino, M., Zingarelli, A., Abdelsamad, A. Y., Abo Shaera, E. S., Afshar, M. S., Agatiello, C., Aguiar, P., Ahmad, A. M., Akin, I., Alameda, M., Alegria-Barrero, E., Alejos, R., Alkhashab, K., Alkutshan, R. S. A., Almorraweh, A., Altnji, I., Alvarez Iorio, C., Anchidin, O., Angel, J., Antonopoulos, A., Apshilava, G., Arana, C., Ashikaga, T., Assomull, R., Atef, S. Z., Azmus, A. D., Azzalini, L., Azzouz, A., Baglioni, P., Bampas, G., Basil, M. P., Besh, D., Bhushan Sharm, A., Bien Hsien, H., Bihui, L., Bing-Chen, L., Biryukov, S., Blatt, A., Bocchi, E., Boghdady, A., Bonarjee, V. V. S., Bosnjak, I., Bravo Baptista, S., Brinckman, S. L., Buchter, B., Burzotta, F., Cacucci, M., Cagliyan, C. E., Cernetti, C., Chavez Mizraym, R., Choo, W. S., Choudhury, R., Cicco, N., Cisneros Clavijo, P., Citaku, H., Collet, J. P., Consuegra-Sanchez, L., Conte, M., Corral, J. M., Damonte, A., Dangoisse, V., Dastani, M., Della Rosa, F., Deora, S., Devadathan, S., Dharma, S., Di Giorgio, A., Diez, J. L., Dinesha, B., Duplancic, D., El Behwashi, M. F., Elghawaby, H., Elshahawy, O., Eskola, M. J., Etman, A., Eun Gyu, L., Fabiano, L., Facta, A., Fan, Y., Fang-Yang, H., Farag, E., Fathi, Y., Fazeli, N., Federico, P., Fereidoun, M. Z., Fernandez-Nofrerias, E., Flensted Lassen, J., Flessas, D., Fouad, H., Franco-Pelaez, J. A., Fu, Q., Furtado, R., Gadepalli, R., Gallino, R., Gasparetto, V., Gentiletti, A., Gholoobi, A., Ghosh, A. K., Gkizas, S., Golchha, S. K., Goncharov, A., Gossl, M., Gotberg, M., Greco, F., Grundeken, M. J., Gupta, D., Gupta, S., Guray, U., Hahalis, G., Hakim Vista, J., Hamid, M. A., Hammoudeh, A., Hasan, A. R. I., Hatsumura, F. E., Heintzen, M. P., Helal, T., Hetherington, S., Hewarathna, U. I., Hioki, H., Hissein, F., Ho-Ping, Y., Homs, S., Huber, K., Ibarra, F. M., Ielasi, A., Ipek, E., Jambunathan, R., Jamshidi, P., Jarrad, I., Javier, W., Jensen, J., Jimenez-Quevedo, P., Kalpak, O., Kan, J., Kanaan, T., Kao, D. H. M., Karamfiloff, K., Karegren, A., Karjalainen, P. P., Kasabov, R., Katsimagklis, G. D., Kaul, U., Khan, A., Kiemeneij, E., Kiviniemi, T., Kleiban, A., Komiyama, N., Konteva, M., Koshy, G., Krepsky, A. M., Kuljit, S., Kulkarni, P., Kumar, V., Kuznetsov, I., Lai, G., Lateef, M. A., Lawand, S., Le Hong, T., Lettieri, C., Levy, G., Lindvall, P., Maitra, A., Makowski, M., Mamas, M. A., Mandal, S. C., Mangalanandan, P., Marin, R., Mashhadi, M., Matsukage, T., Meier, B., Milosavljevic, B., Miro, S. S., Mitov, A., Moeriel, M., Moguel, R., Mohanty, A., Montalescot, G., Morsdorf, W., Moscato, F., Muniz, A., Muraglia, S., Myc, J., Nada, A., Nair, P., Namazi, M. H., Naraghipour, F., Nguyen, Q. N., Nicosia, A., Nikas, D., Ober, M., Ocaranza-Sanchez, R., Olivecrona, G., Pahlajani, D., Pandey, B. P., Parma, A., Parma, R., Patsilinakos, S. P., Pattam, J., Peddi, S., Perez, P. R., Peruga, J. Z., Pescoller, F., Petrov, I., Piatti, L., Pico-Aracil, F., Pina, J., Piroth, Z., Popa, V., Pourbehi, M. R., Pradhan, A. K., Prida, X. E., Purohit, B. V., Pyun, W. B., Quang Hung, D., Rada, I., Rafizadeh, O., Rahman, M. A., Rai, L., Ramsewak, A., Ravindran, R., Rodriguez De Leiras, O. S., Rodriguez Esteban, M., Roque Figueira, H., Saket, A., Sakhov, O., Saktheeswaran, M. K., Salachas, A., Sallam, A., Sampaolesi, A., Samy, A., Sanchis, J., Santaera, O., Santarelli, A., Santharaj, W. S., Sarango, B., Satheesh, S., Schmitz, T., Schuhlen, H., Seewoosagur, R., Segev, A., Seisembekov, V., Semitko, S., Sengottuvelu, G., Sepulveda Varela, P., Sethi, A., Sharma, A., Sharma, R. K., Shi, Hy., Simsek, M. A., Siqueira, B., Skalidis, E., Slawin, J., Sorokhtey, L., Spaulding, C., Srinivas, B., Srinivasan, M., Stakos, D., Stojkovic, S., Tacoy, G., Tawade, M., Tiecco, F., Tondi, S., Torresani, E. M., Tousek, P., Tran, T., Trantalis, G., Triantafyllou, K., Trivedi, R., Trivisonno, A., Tsui, K. L., Turkoglu, C., Tzung-Dau, W., Ueno, H., Urban, U., Uretsky, B. F., Uscumlic, A., Venugopal, V., Verney, R., Vilar, J. V., Villacorta, V. G., Vishwanath, R., Vlachojannis, G. J., Vlachojannis, M., Vlad, V., Von Birgelen, C., Vukcevic, V., Wahab, A., Waksman, R., Wei-Wen, L., Weisz, G., Whittaker, A., Yadav, A., Yokoi, Y., Zacharoulis, A., Zahran, M., Zamani, J., Ziakas, A., Zimmermann, J. P., and Cardiology

Subjects
Hirudin, Percutaneous, Antithrombin, medicine.medical_treatment, Psychological intervention, 030204 cardiovascular system & hematology, medical, 0302 clinical medicine, Peptide Fragment, Surveys and Questionnaires, Surveys and Questionnaire, Medicine, Bivalirudin, 030212 general & internal medicine, Societies, Medical, Transradial, Anticoagulant, Hirudins, Middle Aged, Recombinant Protein, Recombinant Proteins, Femoral Artery, Radial Artery, Cardiology, acute coronary syndrome, bivalirudin, transradial, adult, antithrombins, cardiology, femoral artery, hirudins, humans, middle aged, peptide fragments, percutaneous coronary intervention, recombinant proteins, societies, medical, surveys and questionnaires, attitude of health personnel, radial artery, Acute coronary syndrome, Cardiology and Cardiovascular Medicine, Human, medicine.drug, Adult, medicine.medical_specialty, Attitude of Health Personnel, medicine.drug_class, MEDLINE, Antithrombins, 03 medical and health sciences, societies, Percutaneous Coronary Intervention, Internal medicine, Humans, Acute Coronary Syndrome, Peptide Fragments, Management of acute coronary syndrome, business.industry, Percutaneous coronary intervention, medicine.disease, business
Abstract

AIMS Our aim was to report on a survey initiated by the European Association of Percutaneous Cardiovascular Interventions (EAPCI) collecting the opinion of the cardiology community on the invasive management of acute coronary syndrome (ACS), before and after the MATRIX trial presentation at the American College of Cardiology (ACC) 2015 Scientific Sessions. METHODS AND RESULTS A web-based survey was distributed to all individuals registered on the EuroIntervention mailing list (n=15,200). A total of 572 and 763 physicians responded to the pre- and post-ACC survey, respectively. The radial approach emerged as the preferable access site for ACS patients undergoing invasive management with roughly every other responder interpreting the evidence for mortality benefit as definitive and calling for a guidelines upgrade to class I. The most frequently preferred anticoagulant in ACS patients remains unfractionated heparin (UFH), due to higher costs and greater perceived thrombotic risks associated with bivalirudin. However, more than a quarter of participants declared the use of bivalirudin would increase after MATRIX. CONCLUSIONS The MATRIX trial reinforced the evidence for a causal association between bleeding and mortality and triggered consensus on the superiority of the radial versus femoral approach. The belief that bivalirudin mitigates bleeding risk is common, but UFH still remains the preferred anticoagulant based on lower costs and thrombotic risks.

Published
2016
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59. Nucleosynthesis in asymptototic giant branch stars: relevance for galactic enrichment and solar system formation

Author

Busso, M., Gallino, R., and Wasserburg, G.J.

Subjects
Astrophysics -- Research, Stars, Supernovae -- Research, Red giants -- Spectra, Nucleosynthesis -- Research, Solar system -- Research, Dwarf stars -- Research, Astronomy, Physics
Abstract

Nucleosynthesis of asymptotic giant branch (AGB) stars is reviewed with an outline of development of theoretical models and their relationship to observations. New high-resolution codes with improved opacities are the focus. Recently these codes accounted for the third dredge-up bringing the possibility of understanding low-luminosity C stars enriched in s-elements as the expected outcome of AGB evolution. Galactic enrichment and solar system formation.

Published
1999

61. Measurement of the 151Sm(n, γ) 152Sm cross section at n_TOF

Author

Marrone, S., Abbondanno, U., Aerts, G., Alvarez-Velarde, F., Álvarez-Pol, H., Andriamonje, S., Andrzejewski, J., Badurek, G., Baumann, P., Bečvář, F., Benlliure, J., Berthoumieux, E., Calviño, F., Cano-Ott, D., Capote, R., Cennini, P., Chepel, V., Chiaveri, E., Colonna, N., Cortes, G., Cortina, D., Couture, A., Cox, J., Dababneh, S., Dahlfors, M., David, S., Dolfini, R., Domingo-Pardo, C., Duran, I., Embid-Segura, M., Ferrant, L., Ferrari, A., Ferreira-Marques, R., Frais-Koelbl, H., Furman, W., Goncalves, I., Gallino, R., Gonzalez-Romero, E., Goverdovski, A., Gramegna, F., Griesmayer, E., Gunsing, F., Haas, B., Haight, R., Heil, M., Herrera-Martinez, A., Isaev, S., Jericha, E., Käppeler, F., Kadi, Y., Karadimos, D., Kerveno, M., Ketlerov, V., Koehler, P., Konovalov, V., Krtička, M., Lamboudis, C., Leeb, H., Lindote, A., Lopes, I., Lozano, M., Lukic, S., Marganiec, J., Martinez-Val, J., Mastinu, P., Mengoni, A., Milazzo, P.M., Molina-Coballes, A., Moreau, C., Mosconi, M., Neves, F., Oberhummer, H., O'Brien, S., Pancin, J., Papaevangelou, T., Paradela, C., Pavlik, A., Pavlopoulos, P., Perlado, J.M., Perrot, L., Pignatari, M., Flag, R., Plompen, A., Plukis, A., Poch, A., Policarpo, A., Pretel, C., Quesada, J., Raman, S., Rapp, W., Rauscher, T., Reifarth, R., Rosetti, M., Rubbia, C., Rudolf, G., Rullhusen, P., Salgado, J., Scares, J.C., Stephan, C., Tagliente, G., Tain, J.L., Tassan-Got, L., Tavora, L., Terlizzi, R., Vannini, G., Vaz, P., Ventura, A., Villamarin, D., Vincente, M.C., Vlachoudis, V., Voss, F., Wendler, H., Wiescher, M., and Wisshak, K.

Published
2005
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62. Neutron capture cross section measurements for nuclear astrophysics at CERN n_TOF

Author

Abbondanno, U., Aerts, G., Alvarez-Velarde, F., Álvarez-Pol, H., Andriamonje, S., Andrzejewski, J., Badurek, G., Baumann, P., Bečvář, F., Benlliure, J., Berthoumieux, E., Calviño, F., Cano-Ott, D., Capote, R., Cennini, P., Chepel, V., Chiaveri, E., Colonna, N., Cortes, G., Cortina, D., Couture, A., Cox, J., Dababneh, S., Dahlfors, M., David, S., Dolfini, R., Domingo-Pardo, C., Duran, I., Embid-Segura, M., Ferrant, L., Ferrari, A., Ferreira-Marques, R., Frais-Kölbl, H., Furman, W., Goncalves, I., Gallino, R., Gonzalez-Romero, E., Goverdovski, A., Gramegna, F., Griesmayer, E., Gunsing, F., Haas, B., Haight, R., Heil, M., Herrera-Martinez, A., Isaev, S., Jericha, E., Käppeler, F., Kadi, Y., Karadimos, D., Kerveno, M., Ketlerov, V., Koehler, P., Konovalov, V., Krtička, M., Lamboudis, C., Leeb, H., Lindote, A., Lopes, I., Lorusso, G., Lozano, M., Lukic, S., Marganiec, J., Marrone, S., Martinez-Val, J., Mastinu, P., Mengoni, A., Milazzo, P.M., Molina-Coballes, A., Moreau, C., Mosconi, M., Neves, F., Oberhummer, H., O'Brien, S., Pancin, J., Papaevangelou, T., Paradela, C., Pavlik, A., Pavlopoulos, P., Perlado, J.M., Perrot, L., Pignatari, M., Plag, R., Plompen, A., Plukis, A., Poch, A., Policarpo, A., Pretel, C., Quesada, J., Rapp, W., Rauscher, T., Reifarth, R., Rosetti, M., Rubbia, C., Rudolf, G., Rullhusen, P., Salgado, J., Soares, J.C., Stephan, C., Tagliente, G., Tain, J.L., Tassan-Got, L., Tavora, L., Terlizzi, R., Vannini, G., Vaz, P., Ventura, A., Villamarin, D., Vincente, M.C., Vlachoudis, V., Voss, F., Wendler, H., Wiescher, M., and Wisshak, K.

Published
2005
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64. Measurements of the 90,91,92,94,96Zr( n, γ) cross-sections at n_TOF

Author

Tagliente, G., Abbondanno, U., Aerts, G., Alvarez-Velarde, F., Álvarez-Pol, H., Andriamonje, S., Andrzejewski, J., Badurek, G., Baumann, P., Bečvář, F., Benlliure, J., Berthoumieux, E., Calviño, F., Cano-Ott, D., Capote, R., Cennini, P., Chepel, V., Chiaveri, E., Colonna, N., Cortes, G., Cortina, D., Couture, A., Cox, J., Dababneh, S., Dahlfors, M., David, S., Dolfini, R., Domingo-Pardo, C., Duran, I., Embid-Segura, M., Ferrant, L., Ferrari, A., Ferreira-Marques, R., Frais-Köelbl, H., Furman, W., Goncalves, I., Gallino, R., Gonzalez-Romero, E., Goverdovski, A., Gramegna, F., Griesmayer, E., Gunsing, F., Haas, B., Haight, R., Heil, M., Herrera-Martinez, A., Isaev, S., Jericha, E., Käppeler, F., Kadi, Y., Karadimos, D., Kerveno, M., Ketlerov, V., Koehler, P., Konovalov, V., Krtička, M., Lamboudis, C., Leeb, H., Lindote, A., Lopes, I., Lorusso, G., Lozano, M., Lukic, S., Marganiec, J., Marrone, S., Martinez-Val, J., Mastinu, P., Mengoni, A., Milazzo, P.M., Molina-Coballes, A., Moreau, C., Mosconi, M., Neves, F., Oberhummer, H., O'Brien, S., Pancin, J., Papaevangelou, T., Paradela, C., Pavlik, A., Pavlopoulos, P., Perlado, J.M., Perrot, L., Pignatari, M., Plag, R., Plompen, A., Plukis, A., Poch, A., Policarpo, A., Pretel, C., Quesada, J., Rapp, W., Rauscher, T., Reifarth, R., Rosetti, M., Rubbia, C., Rudolf, G., Rullhusen, P., Salgado, J., Soares, J.C., Stephan, C., Tain, J.L., Tassan-Got, L., Tavora, L., Terlizzi, R., Vannini, G., Vaz, P., Ventura, A., Villamarin, D., Vincente, M.C., Vlachoudis, V., Voss, F., Wendler, H., Wiescher, M., and Wisshak, K.

Published
2005
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72. Presolar SiC of Type Y: Origin from Low-Metallicity Asymptotic Giant Branch Stars

Author

Amari, S, Nittler, L. R, Zinner, E, Gallino R, Lugaro, M, and Lewis, R. S

Subjects
Lunar And Planetary Science And Exploration
Abstract

Carbon and Si isotopic ratios of SiC grains of type Y point to an origin in AGB stars of lower-than-solar metallicity. Comparison with model calculations indicate that stars with metallicity Z = 0.01 and 3-5 solar masses best account for the experimental data.

Published
2000

81. Injection of freshly synthesized Ca-41 in the early solar nebula by an asymptotic giant branch star

Author

Wasserburg, G. J, Gallino, R, Busso, M, Goswami, J. N, and Raiteri, C. M

Subjects
Astrophysics
Abstract

We show that ejecta from the envelope of one asymptotic giant branch star of M is approximately 3 solar mass may account for many of the short-lived nuclei in the early solar system and also for the recent evidence of the presence of Ca-41 (bar-tau(sub 41) = 1.50 x 10(exp 5) yr) in early solar nebular condensates. This would require that the injection into the protosolar molecular cloud took place within a narrow time interval of (5-7) x 10(exp 5) yr before the formation of the solar system. If true, this places extremely tight constraints on the whole process of injection mixing and collapse. The timescales for both Ca-41 and Al-26 require that the placental medium be a dense molecular cloud (2 x 10(exp 3) -8 x 10(exp 3( H/cc). If the observed residual Ca-41 is instead produced by a proton bombardment mechanism within the early solar system, similar to what appears necessary to explain Mn-53, then the time interval is relaxed but would still be (1-2) x 10(exp 6) yr from consideration of Al-26.

Published
1995
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82. Asymptotic Giant Branch stars as a source of short-lived radioactive nuclei in the solar nebula

Author

Wasserburg, G. J, Busso, M, Gallino, R, and Raiteri, C. M

Subjects
Astrophysics
Abstract

We carried out a theoretical evaluation of the contribution of Asymptotic Giant Branch (AGB) stars to some short-lived (10(exp 6) less than or equal to Tau-bar less than or equal to 2 x 10(exp 7) yr) isotopes in the Interstellar Medium (ISM) and in the early solar system using stellar model calculations for thermally pulsing evolutionary phases of low-mass stars. The yields of s-process nuclei in the convective He-shell for different neutron exposures tau(sub 0) were obtained, and AGB stars were shown to produce several radioactive nuclei (especially Pd-107, Pb-205, Fe-60, Zr-93, Tc-99, Cs-135, and Hf-182) in diferent amounts. Assuming either contamination of the solar nebula from a single AGB star or models for continuous injection and mixing from many stars into the ISM, we calculate the ratios of radioactive to stable nuclei at the epoch of the Sun's formation. The dilution factor between the AGB ejecta and the early solar system matter is obtained by matching the observed Pd-107/Pd-108 and depends on the value of tau(sub 0). It is found that small masses M(sub He) of He-shell material (10(exp -4)-10(exp -7) solar mass) enriched in s-process nuclei are sufficient to contaminate 1 solar mass of the ISM to produce the Pd-107 found in the early solar system. Predictions are made for all of the other radioactive isotopes. The optimal model to explain several observed radioactive species at different states of the proto-solar nebula involves a single AGB star with a low neutron exposure (tau(sub 0) = 0.03 mbarn(sup -1)) which contaminated the cloud with a dilution factor of M(sub He)/solar mass approximately 1.5 x 10(exp -4). This will also contribute newly synthesized stable s-process nuclei in the amount of approximately 10(exp -4) of their abundances already present in the proto-solar cloud. Variations in the degree of homogenization (approximately 30%) of the injected material may account for some of the small general isotopic anomalies found in meteorites. It is also found that Fe-60 is produced in small but significant quantities that may be sufficient to explain the observations if the time elapsed delta from the contamination of the ISM to the formation of protoplanetary bodies is not higher than delta = 5 x 10(exp 6) yr. If delta is longer, up to 10 x 10(exp 6) yr, this would require the single AGB star to experience enhanced neutron densities (n(sub n) approximately 3 x 10(exp 9)n/cu cm) in the s-processing zone in order to compensate for the branching at Fe-59. The alternative model of long-term continuous ejection of matter from many AGB stars does not appear to match the observations. We also estimate the Al-26 production from the H-shell and find that the Al-26 abundance in the early solar system may be readily explained in a self-consistent manner. Moreover, Al-26 from AGB stars may contribute substantially to the galactic Al-26 gamma-source, while no significant gamma-flux from Co-60 (deriving from Fe-60 decay) is to be expected.

Published
1994
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83. AGB stars as a source of short-lived radioactive nuclei in the solar nebula

Author

Wasserburg, G. J, Gallino, R, Busso, M, and Raiteri, C. M

Subjects
Solar Physics
Abstract

The purpose is to estimate the possible contribution of some short-lived nuclei to the early solar nebula from asymptotic giant branch (AGB) sources. Low mass (1 to 3 solar mass) AGB stars appear to provide a site for synthesis of the main s process component for solar system material with an exponential distribution of neutron irradiations varies as exp(-tau/tau(sub 0)) (where tau is the time integrated neutron flux with a mean neutron exposure tau(sub 0)) for solar abundances with tau(sub 0) = 0.28 mb(sup -1). Previous workers estimated the synthesis of key short-lived nuclei which might be produced in AGB stars. While these calculations exhibit the basic characteristics of nuclei production by neutron exposure, there is need for a self-consistent calculation that follows AGB evolution and takes into account the net production from a star and dilution with the cloud medium. Many of the general approaches and the conclusions arrived at were presented earlier by Cameron. The production of nuclei for a star of 1.5 solar mass during the thermal pulsing of the AGB phase was evaluated. Calculations were done for a series of thermal pulses with tau(sub 0) = 0.12 and 0.28 mb(sup -1). These pulses involve s nucleosynthesis in the burning shell at the base of the He zone followed by the ignition of the H burning shell at the top of the He zone. After about 10-15 cycles the abundances of the various nuclei in the He zone become constant. Computations of the abundances of all nuclei in the He zone were made following Gallino. The mass of the solar nebula was considered to consist of some initial material of approximately solar composition plus some contributions from AGB stars. The ratios of the masses required from the AGB He burning zone to the ISM necessary to produce the observed value of Pd-107/Pd-108 in the early solar system were calculated and this dilution factor was applied to all other relevant nuclei.

Published
1993

85. Neutron-induced fission cross section of Np237 in the keV to MeV range at the CERN n_TOF facility

Author

Diakaki, M, Karadimos, D, Vlastou, R, Kokkoris, M, Demetriou, P, Skordis, E, Tsinganis, A, Abbondanno, U, Aerts, G, Álvarez, H, Alvarez-Velarde, F, Andriamonje, S, Andrzejewski, J, Assimakopoulos, P, Audouin, L, Badurek, G, Baumann, P, Bečvář, F, Berthoumieux, E, Calviani, M, Calviño, F, Cano-Ott, D, Capote, R, Carrillo de Albornoz, A, Cennini, P, Chepel, V, Chiaveri, E, Colonna, N, Cortes, G, Couture, A, Cox, J, David, S, Dolfini, R, Domingo-Pardo, C, Dorochenko, A, Dridi, W, Duran, I, Eleftheriadis, Ch, Embid-Segura, M, Ferrant, L, Ferrari, A, Ferreira-Marques, R, Fitzpatrick, L, Frais-Koelbl, H, Fuji, K, Furman, W, Goncalves, I, Gallino, R, Gonzalez-Romero, E, Goverdovski, A, Gramegna, F, Griesmayer, E, Guerrero, C, Gunsing, F, Haas, B, Haight, R, Heil, M, Herrera-Martinez, A, Igashira, M, Ioannidis, K, Isaev, S, Jericha, E, Kadi, Y, Käppeler, F, Karamanis, D, Kerveno, M, Ketlerov, V, Koehler, P, Kolokolov, D, Konovalov, V, Krtička, M, Lamboudis, C, Leeb, H, Lindote, A, Lopes, I, Lozano, M, Lukic, S, Marganiec, J, Marques, L, Marrone, S, Massimi, C, Mastinu, P, Mengoni, A, Milazzo, P M, Moreau, C, Mosconi, M, Neves, F, Oberhummer, H, O'Brien, S, Oshima, M, Pancin, J, Papadopoulos, C, Paradela, C, Patronis, N, Pavlik, A, Pavlopoulos, P, Perrot, L, Plag, R, Plompen, A, Plukis, A, Poch, A, Pretel, C, Quesada, J, Rauscher, T, Reifarth, R, Rosetti, M, Rubbia, C, Rudolf, G, Rullhusen, P, Salgado, J, Sarchiapone, L, Savvidis, I, Sedysheva, M, Stamoulis, K, Stephan, C, Tagliente, G, Tain, J L, Tassan-Got, L, Tavora, L, Terlizzi, R, Vannini, G, Vaz, P, Ventura, A, Villamarin, D, Vincente, M C, Vlachoudis, V, Voss, F, Wendler, H, Wiescher, M, and Wisshak, K

Subjects
Nuclear Physics - Experiment, Nuclear Experiment
Abstract

The neutron-induced fission cross section of Np237 was experimentally determined at the high-resolution and high-intensity facility n_TOF, at CERN, in the energy range 100 keV to 9 MeV, using the U235(n,f) and U238(n,f) cross section standards below and above 2 MeV, respectively. A fast ionization chamber was used in order to detect the fission fragments from the reactions and the targets were characterized as far as their mass and homogeneity are concerned by means of α spectroscopy and Rutherford backscattering spectroscopy respectively. Theoretical calculations within the Hauser-Feshbach formalism have been performed, employing the empire code, and the model parameters were tuned in order to successfully reproduce the experimental fission cross-sectional data and simultaneously all the competing reaction channels.

Published
2016

88. Zirconium isotope evidence for the heterogeneous distribution of s-process materials in the solar system

Author

Akram, W., Schönbächler, M., Bisterzo, S., and Gallino, R.

Subjects
Geochemistry and Petrology
Abstract

A growing number of elements show well-resolved nucleosynthetic isotope anomalies in bulk-rock samples of solar system materials. In order to establish the occurrence and extent of such isotopic heterogeneities in Zr, and to investigate the origin of the widespread heterogeneities in our solar system, new high-precision Zr isotope data are reported for a range of primitive and differentiated meteorites. The majority of the carbonaceous chondrites (CV, CM, CO, CK) display variable ε96Zr values (⩽1.4) relative to the Earth. The data indicate the heterogeneous distribution of 96Zr-rich CAIs in these meteorites, which sampled supernova (SN) material that was likely synthesized by charged-particle reactions or neutron-captures. Other carbonaceous chondrites (CI, CB, CR), ordinary chondrites and eucrites display variable, well-resolved 96Zr excesses correlated with potential, not clearly resolved variations in 91Zr relative to the bulk–Earth and enstatite chondrites. This tentative correlation is supported by nucleosynthetic models and provides evidence for variable contributions of average solar system s-process material to different regions of the solar system, with the Earth representing the most s-process enriched material. New s-process model calculations indicate that this s-process component was produced in both low and intermediate mass asymptotic giant branch (AGB) stars. The isotopic heterogeneity pattern is different to the s-process signature resolved in a previous Zr leaching experiment, which was attributed to low mass AGB stars. The bulk-rock heterogeneity requires several nucleosynthetic sources, and therefore opposes the theory of the injection of material from a single source (e.g., supernova, AGB star) and argues for a selective dust-sorting mechanism within the solar nebula. Thermal processing of labile carrier phases is considered and, if correct, necessitates the destruction and removal of non-s-process material from the innermost solar system. New Zr isotope data on mineral separates and a fusion crust sample from chondrites indicate that this non-s-process material could be silicates., Geochimica et Cosmochimica Acta, 165, ISSN:0016-7037, ISSN:1872-9533

Published
2015

89. Nuclear Astrophysics at the n_TOF facility, CERN

Author

Tagliente, G, Abbondanno, U, Aerts, G, Alvarez, H, Alvarez-Velarde, F, Andriamonje, S, Andrzejewski, J, Audouin, L, Badurek, G, Baumann, P, Bečvář, F, Belloni, F, Berthoumieux, E, Bisterzo, S, Calviño, F, Calviani, M, Cano-Ott, D, Capote, R, Carrapiço, C, Cennini, P, Chepel, V, Chiaveri, E, Colonna, N, Cortes, G, Couture, A, Cox, J, Dahlfors, M, David, S, Dillman, I, Domingo-Pardo, C, Dridi, W, Duran, I, Eleftheriadis, C, Embid-Segura, M, Ferrari, A, Ferreira-Marques, R, Fujii, K, Furman, W, Gallino, R, Goncalves, I, Gonzalez-Romero, E, Gramegna, F, Guerrero, C, Gunsing, F, Haas, B, Haight, R, Heil, M, Herrera-Martinez, A, Igashira, M, Jericha, E, Käppeler, F, Kadi, Y, Karadimos, D, Karamanis, D, Kerveno, M, Koehler, P, Kossionides, E, Krtička, M, Leeb, H, Lindote, A, Lopes, I, Lozano, M, Lukic, S, Marganiec, J, Marrone,S, Martinez, T, Massimi, C, Mastinu, P, Mengoni, A, Milazzo, P M, Mosconi, M, Neves, F, Oberhummer, H, Pancin, J, Papachris-todoulou, C, Papadopoulos, C, Paradela, C, Patronis, N, Pavlik, A, Pavlopoulos, P, Perrot, L, Pigni, M T, Plag, R, Plompen, A, Plukis, A, Poch, A, Praena, J, Pretel, C, Quesada, J, Rauscher, T, Reifarth, R, Rubbia, C, Rudolf, G, Rullhusen, P, Salgado, J, Santos, C, Sarchiapone, L, Savvidis, I, Stephan, C, Tain, J L, Tassan-Got, L, Tavora, L, Terlizzi, R, Vannini, G, Vaz, P, Ventura, A, Villamarin, A, Vincente, M C, Vlachoudis, V, Vlastou, V, Voss, F, Walter, F, Wendler, H, Wiescher, M, and Wisshak, K

Subjects
Nuclear Physics - Experiment
Published
2015

91. Stellar neutron capture cross sections of Ne20,21,22

Author

Heil, M, Plag, R, Uberseder, E, Gallino, R, Bisterzo, S, Juseviciute, A, Käppeler, F, Lederer, C, Mengoni, A, and Pignatari, M

Subjects
Astrophysics and Astronomy, Nuclear Physics - Theory, Nuclear Astrophysics, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

The stellar (n,γ) cross sections of the Ne isotopes are important for a number of astrophysical quests, i.e., for the interpretation of abundance patterns in presolar material or with respect to the s-process neutron balance in red giant stars. This paper presents resonance studies of experimental data in the keV range, which had not been fully analyzed before. The analyses were carried out with the R-matrix code sammy. With these results for the resonant part and by adding the components due to direct radiative capture, improved Maxwellian-averaged cross sections (MACS) could be determined. At kT=30keV thermal energy we obtain MACS values of 240±29,1263±160, and 53.2±2.7 μbarn for Ne20,Ne21, and Ne22, respectively. In earlier work the stellar rates of Ne20 and Ne21 had been grossly overestimated. Ne22 and Ne20 are significant neutron poisons for the s process in stars because their very small MACS values are compensated by their large abundances.

Published
2014

98. Nuclear astrophysics at n_TOF, CERN

Author

Tagliente, G, Abbondanno, U, Aerts, G, Alvarez, H, Alvarez-Velarde, F, Andriamonje, S, Andrzejewski, J, Audouin, L, Badurek, G, Baumann, P, Bečvář, F, Belloni, F, Berthoumieux, E, Bisterzo, S, Calviño, F, Calviani, M, Cano-Ott, D, Capote, R, Carrapiço, C, Cennini, P, Chepel, V, Chiaveri, E, Colonna, N, Cortes, G, Couture, A, Cox, J, Dahlfors, M, David, S, Dillman, I, Domingo-Pardo, C, Dridi, W, Duran, I, Eleftheriadis, C, Embid-Segura, M, Ferrari, A, Ferreira-Marques, R, Fujii, K, Furman, W, Gallino, R, Goncalves, I, Gonzalez-Romero, E, Gramegna, F, Guerrero, C, Gunsing, F, Haas, B, Haight, R, Heil, M, Herrera-Martinez, A, Igashira, M, Jericha, E, Käppeler, F, Kadi, Y, Karadimos, D, Karamanis, D, Kerveno, M, Koehler, P, Kossionides, E, Krtička, M, Leeb, H, Lindote, A, Lopes, I, Lozano, M, Lukic, S, Marganiec, J, Marrone, S, Martinez, T, Massimi, C, Mastinu, P, Mengoni, A, Milazzo, P M, Mosconi, M, Neves, F, Oberhummer, H, Pancin, J, Papachristodoulou, C, Papadopoulos, C, Paradela, C, Patronis, N, Pavlik, A, Pavlopoulos, P, Perrot, L, Pigni, M T, Plag, R, Plompen, A, Plukis, A, Poch, A, Praena, J, Pretel, C, Quesada, J, Rauscher, T, Reifarth, R, Rubbia, C, Rudolf, G, Rullhusen, P, Salgado, J, Santos, C, Sarchiapone, L, Savvidis, I, Stephan, C, Tain, J L, Tassan-Got, L, Tavora, L, Terlizzi, R, Vannini, G, Vaz, P, Ventura, A, Villamarin, D, Vincente, M C, Vlachoudis, V, Vlastou, R, Voss, F, Walter, S, Wendler, H, Wiescher, M, and Wisshak, K

Subjects
Nuclear Physics - Experiment
Published
2012

99. Resonance neutron-capture cross sections of stable magnesium isotopes and their astrophysical implications

Author

Massimi, C., Koehler, P., Bisterzo, S., Colonna, N., Gallino, R., Gunsing, F., Lorusso, G., Mengoni, A., Pignatari, M., Vannini, G., Papachristodoulou, C., Rubbia, C., O Brien, S., Pavlik, A., Oshima, M., Pancin, J., Pavlopoulos, P., Perrot, L., Pigni, M. T., Plukis, A., Poch, A., Villamarin, D., Praena, J., Aerts, G., Pretel, C., Quesada, J., Rauscher, T., Reifarth, R., Assimakopoulos, P., Rockefeller, G., Rudolf, G., Salgado, J., Badurek, G., Santos, C., Sarchiapone, L., Sarmento, R., Savvidis, I., Audouin, L., Stephan, C., Tagliente, G., Tain, J. L., Tassan-Got, L., Tavora, L., Cano-Ott, D., Terlizzi, R., Vaz, P., Ventura, A., Vlachoudis, V., Vlastou, R., Voss, F., Walter, S., Wendler, H., Wiescher, M., Wisshak, K., Dridi, W., Andriamonje, S., Andrzejewski, J., Barbagallo, M., Capote, R., Baumann, P., Belloni, F., Bennett, M., Berthoumieux, E., Calviani, M., Griesmayer, E., Duran, I., Carrillo de Albornoz, A., Cennini, P., Chepel, V., Chiaveri, E., Cortes, G., Couture, A., Guerrero, C., Isaev, S., Cox, J., Dahlfors, M., Eleftheriadis, C., David, S., Dillmann, I., Dolfini, R., Domingo-Pardo, C., Embid-Segura, M., Papadopoulos, C., Haas, B., Ferrant, L., Ferrari, A., Ferreira-Marques, R., Fitzpatrick, L., Lederer, C., Frais-Koelbl, H., Fujii, K., Furman, W., Goncalves, I., Jericha, E., Goverdovski, A., Haight, R., Gramegna, F., Heil, M., Herrera-Martinez, A., Lindote, A., Herwig, F., Hirschi, R., Igashira, M., Kadi, Y., Karadimos, D., Karamanis, D., Kerveno, M., Ketlerov, V., Konovalov, V., Kopecky, S., Lopes, I., Plag, R., Kossionides, E., Paradela, C., Lampoudis, C., Leeb, H., Losito, R., Lozano, M., Lukic, S., Plompen, A., Marganiec, J., Marques, L., Patronis, N., Rosetti, M., Marrone, S., Mastinu, P., Mendoza, E., Milazzo, P. M., Moreau, C., Mosconi, M., Abbondanno, U., Neves, F., and Oberhummer, H.

Abstract

Physical Review C

Published
2012

100. Neutron capture on Zr-94: Resonance parameters and Maxwellian-averaged cross sections

Author

Tagliente, G., Milazzo, P. M., Fujii, K., Abbondanno, U., Aerts, G., Alvarez, H., Alvarez-Velarde, F., Andriamonje, S., Andrzejewski, J., Audouin, L., Badurek, G., Baumann, P., Becvar, F., Belloni, F., Berthoumieux, E., Bisterzo, S., Calvino, F., Calviani, M., Cano-Ott, D., Capote, R., Carrapico, C., Cennini, P., Chepel, V., Chiaveri, E., Colonna, N., Cortes, G., Couture, A., Cox, J., Dahlfors, M., David, S., Dillmann, I., Domingo-Pardo, C., Dridi, W., Duran, I., Eleftheriadis, C., Embid-Segura, M., Ferrari, A., Ferreira-Marques, R., Furman, W., Gallino, R., Goncalves, I., Gonzalez-Romero, E., Gramegna, F., Guerrero, C., Gunsing, F., Haas, B., Haight, R., Heil, M., Herrera-Martinez, A., Jericha, E., Kappeler, F., Kadi, Y., Karadimos, D., Karamanis, D., Kerveno, M., Kossionides, E., Krticka, M., Lamboudis, C., Leeb, H., Lindote, A., Lopes, I., Lozano, M., Lukic, S., Marganiec, J., Marrone, S., Martinez, T., Massimi, C., Mastinu, P., Mengoni, A., Moreau, C., Mosconi, M., Neves, F., Oberhummer, H., O'Brien, S., Pancin, J., Papachristodoulou, C., Papadopoulos, C., Paradela, C., Patronis, N., Pavlik, A., Pavlopoulos, P., Perrot, L., Pigni, M. T., Plag, R., Plompen, A., Plukis, A., Poch, A., Praena, J., Pretel, C., Quesada, J., Rauscher, T., Reifarth, R., Rosetti, M., Rubbia, C., Rudolf, G., Rullhusen, P., Salgado, J., Santos, C., Sarchiapone, L., Savvidis, I., Stephan, C., Tain, J. L., Tassan-Got, L., Tavora, L., Terlizzi, R., Vannini, G., Vaz, P., Ventura, A., Villamarin, D., Vincente, M. C., Vlachoudis, V., Vlastou, R., Voss, F., Walter, S., Wiescher, M., and Wisshak, K.

Subjects
nuclear-data library, n-tof, elements, facility, evolution, nucleosynthesis, zirconium, giant branch stars, system, s-process
Abstract

The neutron capture cross sections of the Zr isotopes play an important role in nucleosynthesis studies. The s-process reaction flow between the Fe seed and the heavier isotopes passes through the neutron magic nucleus Zr-90 and through Zr-91,Zr-92,Zr-93,Zr-94, but only part of the flow extends to Zr-96 because of the branching point at Zr-95. Apart from their effect on the s-process flow, the comparably small isotopic (n, gamma) cross sections make Zr also an interesting structural material for nuclear reactors. The Zr-94 (n, gamma) cross section has been measured with high resolution at the spallation neutron source n_TOF at CERN and resonance parameters are reported up to 60 keV neutron energy. Physical Review C

Published
2011

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