Growth of ultra-high purity NaI(Tl) crystals for dark matter searches
Growth of ultra-high purity NaI(Tl) crystals for dark matter searches
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用于暗物质搜索的超高纯度 NaI(Tl) 晶体的生长
DOI：
10.1103/physrevresearch.2.013223
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发表时间：
2020
影响因子：
4.2
通讯作者：
Ciampi, Guido
中科院分区：
文献类型：
--
作者：
Suerfu, Burkhant;Wada, Masayuki;Peloso, Winston;Souza, Michael;Calaprice, Frank;Tower, Joshua;Ciampi, Guido
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来自 DM-Ice17 的第一个数据
影响因子：
5
作者：
J. Cherwinka;D. Grant;F. Halzen;K. Heeger;L. Hsu;A. Hubbard;A. Hubbard;A. Karle;M. Kauer;M. Kauer;V. Kudryavtsev;C. Macdonald;R. Maruyama;S. Paling;W. Pettus;W. Pettus;Z. Pierpoint;Z. Pierpoint;B. Reilly;B. Reilly;M. Robinson;P. Sandstrom;N. Spooner;S. Telfer;Liang Yang
通讯作者：
Liang Yang
180°C 以上 NaI 中气体热解吸峰的起源
DOI：
--
发表时间：
2009
期刊：
影响因子：
--
作者：
D. Sofronov;K. Kudin;A. Voloshko;A. M. Kudin;O. Shishkin
通讯作者：
O. Shishkin
Polaris：通用、模块化数据采集框架
影响因子：
1.3
作者：
B. Suerfu
通讯作者：
B. Suerfu
影响因子：
5
作者：
R. Agnese;A. Anderson;T. Aralis;T. Aramaki;I. Arnquist;W. Baker;D. Balakishiyeva;D. Barker;
通讯作者：
R. Agnese;A. Anderson;T. Aralis;T. Aramaki;I. Arnquist;W. Baker;D. Balakishiyeva;D. Barker;
影响因子：
3.5
作者：
M. Antonello;E. Barberio;T. Baroncelli;J. Benziger;L. Bignell;I. Bolognino;F. Calaprice;S. Copello;D. D’Angelo;G. D’Imperio;I. Dafinei;G. D. Carlo;M. Diemoz;A. D. Ludovico;A. Duffy;F. Froborg;G. Giovanetti;E. Hoppe;A. Ianni;L. Ioannucci;S. Krishnan;G. Lane;I. Mahmood;A. Mariani;P. McGee;P. Montini;J. Mould;F. Nuti;D. Orlandi;M. Paris;V. Pettinacci;L. Pietrofaccia;D. Prokopovich;S. Rahatlou;N. Rossi;A. Sarbutt;E. Shields;M. Souza;A. Stuchbery;B. Suerfu;C. Tomei;P. Urquijo;C. Vignoli;M. Wada;A. Wallner;A. G. Williams;J. Xu;M. Milano;Milano;Italy;S. O. Physics;The University of Melbourne;Melbourne;Australia;Chemical Engineering Department;Princeton University;Princeton;Nj;USA.;D. Physics;The Australian National University;Canberra;D. Fisica;U. D. S. D. Milano-U.-D.-S.-D.-Milano-102421132;P. Department;I. G. Sasso;Assergi;I. -. G. S. S. Institute-I.-.-G.-S.-S.-Institute-102945001;Infn Roma;Roma;A. J. W. H. C. F. Astrophysics;Centre for Gravitational Astrophysics;Supercomputing;S. U. Technology;I. -. London;High Energy Physics;B. Laboratory;United Kingdom.;P. N. N. Laboratory-P.-N.-N.-Laboratory-7290024;Richland;Wa;The University of Adelaide;Adelaide;South Australia.;S. Roma;Australian Nuclear Science;Technology Organization;Lucas Heights
通讯作者：
M. Antonello;E. Barberio;T. Baroncelli;J. Benziger;L. Bignell;I. Bolognino;F. Calaprice;S. Copello;D. D’Angelo;G. D’Imperio;I. Dafinei;G. D. Carlo;M. Diemoz;A. D. Ludovico;A. Duffy;F. Froborg;G. Giovanetti;E. Hoppe;A. Ianni;L. Ioannucci;S. Krishnan;G. Lane;I. Mahmood;A. Mariani;P. McGee;P. Montini;J. Mould;F. Nuti;D. Orlandi;M. Paris;V. Pettinacci;L. Pietrofaccia;D. Prokopovich;S. Rahatlou;N. Rossi;A. Sarbutt;E. Shields;M. Souza;A. Stuchbery;B. Suerfu;C. Tomei;P. Urquijo;C. Vignoli;M. Wada;A. Wallner;A. G. Williams;J. Xu;M. Milano;Milano;Italy;S. O. Physics;The University of Melbourne;Melbourne;Australia;Chemical Engineering Department;Princeton University;Princeton;Nj;USA.;D. Physics;The Australian National University;Canberra;D. Fisica;U. D. S. D. Milano-U.-D.-S.-D.-Milano-102421132;P. Department;I. G. Sasso;Assergi;I. -. G. S. S. Institute-I.-.-G.-S.-S.-Institute-102945001;Infn Roma;Roma;A. J. W. H. C. F. Astrophysics;Centre for Gravitational Astrophysics;Supercomputing;S. U. Technology;I. -. London;High Energy Physics;B. Laboratory;United Kingdom.;P. N. N. Laboratory-P.-N.-N.-Laboratory-7290024;Richland;Wa;The University of Adelaide;Adelaide;South Australia.;S. Roma;Australian Nuclear Science;Technology Organization;Lucas Heights