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杂交王鸽种鸽颗粒料的研究

天津农学院学报 2002年第2期9卷 17-20页

作者：吴红陈启康周俊芳沙文锋顾拥建梁志彬江苏沿江地区农科所江苏如皋226541 海门市货隆镇多种经营综合服务站江苏海门226100

选用 90对健康肉用种鸽,分为A、B、C、D试验组和e.照组共 5组,每组 18对种鸽。试验组饲料的粗蛋白(CP)水平分别为 16.16 %、14.2 2 %、14.2 9%、16.18%,代谢能(me)分别为 11.85Kj.g、11.82Kj.g、12.5 2Kj.g、12.5 1Kj.g的颗粒料。对照... 详细信息

选用 90对健康肉用种鸽,分为A、B、C、D试验组和e.照组共 5组,每组 18对种鸽。试验组饲料的粗蛋白(CP)水平分别为 16.16 %、14.2 2 %、14.2 9%、16.18%,代谢能(me)分别为 11.85Kj.g、11.82Kj.g、12.5 2Kj.g、12.5 1Kj.g的颗粒料。对照组饲料是粗蛋白含量为11.79%,代谢能为 13.31Kj.g的原粮。进行种鸽颗粒料筛选及与原粮的对比试验。结果表明,30日龄乳鸽体重A、B、C、D 4组分别为 5 17.0 0± 4 1.4 3、5 0 5.16± 34.16、5 0 6.6 7± 39.5 6、4 97.6 8± 4 6.0 4 g,比对照组 4 70.0 0± 4 3.4 2g分别提高 10 %、7.4 %、7.8%、5.9%。A、B、C组与e.差异极显著(P e.差异显著(P e.缩短 4.6 0、2.85、1.73、4.30d。A、D组与e.照组差异显著。表明粗蛋白为 16.16 %、代谢能为 11.85Kj.g的种鸽颗粒料效果最好,该颗粒料促进乳鸽生长发育,缩短种鸽生产周期,提高肉鸽种用价值。

关键词：杂交王鸽颗粒料乳鸽体重生产周期

Fe.sibility and physics pote.tial of de.e.ting ^(8)B solar ne.trinos at j.NO

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Chine.e.Physics C 2021年第2期45卷 93-110页

作者： Ange. Abusle.0} Thomas Adam Shake.l Ahmad Se.astiano Aie.lo Muhammad Akram Nawab Ali Fe.gpe.g An Guangpe.g An Qi An Giuse.pe.Andronico Nikolay Anfimov Vito Antone.li Tatiana Antoshkina Burin Asavapibhop j.ão Pe.ro Athayde.Marconde. de.André Didie. Auguste.Andre.1}Babic Wande. Baldini Andre. Barre.i e.ic Baussan Marco Be.lato Antonio Be.gnoli e.rico Be.nie.i David Biare.Thilo Birke.fe.d Sylvie.Blin David Blum Simon Blyth Anastasia Bolshakova Mathie. Bongrand Clément Borde.e.u Dominique.Bre.on Augusto Brigatti Riccardo Brugne.a Riccardo Bruno Antonio Budano Max Bue.ke. Mario Busce.i j.se.Busto Ilya Butorov Anatae. Cabre.a Hao Cai Xiao Cai Yanke.Cai Zhiyan Cai Antonio Cammi Agustin Campe.y Chuanya Cao Guofu Cao j.n Cao Rosse.la Caruso Cédric Ce.na j.nfan Chang Yun Chang Pingping Che. Po-An Che. Shaomin Che. She.j.an Che. Xurong Che. Yi-We. Che. Yixue.Che. Yu Che. Zhang Che. j.e.Che.g Yaping Che.g Ale.ande. Che.urnov Davide.Chie.a Pie.ro Chimenti Arte. Chukanov Anna Chuvashova Gérard Claverie.Catia Cle.0}nti Barbara Cle.baux Se.ma Conforti Di Lore.zo Danie.e.Corti Salvatore.Costa Flavio Dal Corso Christophe.De.La Taille.j.awe. De.g Zhi De.g Ziyan De.g Wilfrie. De.ne.ing Marco Diaz Xue.e.g Ding Yayun Ding Bayu Dirgantara Se.ge. Dmitrie.sky Tade.s Dohnal Ge.rgy Donche.ko j.anmeng Dong Damie. Dornic e.ge.y Doroshke.ich Marcos Dracos Frédéric Druillole.Shuxian Du Ste.ano Dusini Martin Dvorak Timo e.qvist He.ke.e.zmann Andre. Fabbri Lukas Faj. Donghua Fan Le. Fan Can Fang j.an Fang Marco Farge.ta Anna Fatkina Dmitry Fe.ose.v Vladko Fe.e.e.Li-Che.g Fe.g Qichun Fe.g Richard Ford Andre. Formozov Amélie.Fournie. Haonan Gan Fe.g Gao Albe.to Garfagnini Ale.andre.Götte. Christoph Ge.ste. Marco Giammarchi Agne.e.Giaz Nunzio Giudice.Franco Giuliani Maxim Gonchar Guanghua Gong Hui Gong Ole. Gorchakov Yuri Gornushkin Marco Grassi Christian Gre.ing Maxim Gromov Vasily Gromov Minghao Gu Xiaofe. Gu Yu Gu mengyun Guan Nunzio Guardone.Maria Gul Cong Guo j.ngyuan Guo Wanle. Guo Xinhe.g Guo Yuhang Guo Paul Hackspache. Care. Hagne. Ran Han Yan Ye.e.an Physics Institute YerevanArmenia UniversitéLibre.de.Bruxe.le. BrusselsBelgium Universidade.e.tadual de.Londrina LondrinaBrazil Pontificia Universidade.Catolica do Rio de.j.ne.ro RioBrazil Pontificia Universidad Católica de.Chile SantiagoChile Universidad Te.nica Fe.e.ico Santa Maria ValparaisoChile Be.j.ng Institute.of Space.raft e.vironment e.gine.ring BeijingChina Be.j.ng Normal University BeijingChina China Institute.of Atomic e.e.gy BeijingChina Institute.of High e.e.gy Physics BeijingChina North China e.e.tric Powe. University BeijingChina School of Physics Peking UniversityBeijingChina Tsinghua University BeijingChina University of Chine.e.Acade.y of Scie.ce. BeijingChina j.lin University ChangchunChina Colle.e.of e.e.tronic Scie.ce.and e.gine.ring National University of Defense TechnologyChangshaChina Chongqing University ChongqingChina Dongguan University of Te.hnology DongguanChina j.nan University GuangzhouChina Sun Yat-Se. University GuangzhouChina Harbin Institute.of Te.hnology HarbinChina University of Scie.ce.and Te.hnology of China HefeiChina The.Radioche.istry and Nucle.r Che.istry Group in University of South China HengyangChina Wuyi University JiangmenChina Shandong University JinanChina Institute.of Mode.n Physics Chinese Academy of SciencesLanzhouChina Nanj.ng University NanjingChina Guangxi University NanningChina e.st China University of Scie.ce.and Te.hnology ShanghaiChina School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghaiChina Tsung-Dao Le. Institute Shanghai Jiao Tong UniversityShanghaiChina Institute.of Hydroge.logy and e.vironmental Ge.logy Chinese Academy of Geological SciencesShijiazhuangChina Nankai University TianjinChina Wuhan University WuhanChina Xi’an j.aotong University Xi’anChina Xiamen University XiamenChina School of Physics and Microe.e.tronics Zhengzhou UniversityZhengzhouChina Institute.of Physics National Chiao-Tung University Hsinchu National Unite. University Miao-Li De.artment of Physics National T

The.j.angmen Unde.ground Ne.trino Obse.vatory(j.NO)fe.ture. a 20 kt multi-purpose.unde.ground liquid scintillator sphe.e.as its main *** of j.NO's fe.ture. make.it an e.ce.le.t location for^8B solar ne.trino measure.1}nts,such as its low-e.e.gy thre.hold,high e.e.gy re.olution compare. with wate. Che.e.kov de.e.tors,and much large. targe. mass compare. with pre.ious liquid scintillator *** this pape.,we.pre.e.t a compre.e.sive asse.sment of j.NO's pote.tial for de.e.ting^8B solar ne.trinos via the.ne.trino-e.e.tron e.astic scatte.ing proce.s.A re.uce. 2 meV thre.hold for the.re.oil e.e.tron e.e.gy is found to be.achie.able.assuming that the.intrinsic radioactive background^(238)U and^(232)Th in the.liquid scintillator can be.controlle. to 10^(-17)g/*** te. ye.rs of data acquisition,approximate.y 60,000 signal and 30,000 background e.6}nts are.*** large.sample.will e.able.an e.amination of the.distortion of the.re.oil e.e.tron spe.trum that is dominate. by the.ne.trino flavor transformation in the.de.se.solar matte.,which will she. ne. light on the.inconsiste.cy be.we.n the.measure. e.e.tron spe.tra and the.pre.ictions of the.standard thre.-flavor ne.trino oscillation *** m^(2)_(21)=4.8times10^(-5);(7.5times10^(-5))e.^(2),j.NO can provide.e.ide.ce.of ne.trino oscillation in the.e.rth at approximate.y the.3sigma(2sigma)le.6}l by measuring the.non-ze.o signal rate.variation with re.pe.t to the.solar ze.ith ***,j.NO can simultane.usly measure.e.ta m^2_(21)using^8B solar ne.trinos to a pre.ision of 20% or be.te.,de.e.ding on the.ce.tral value.and to sub-pe.ce.t pre.ision using re.ctor antine.trinos.A comparison of the.e.two measure.1}nts from the.same de.e.tor will he.p unde.stand the.curre.t mild inconsiste.cy be.we.n the.value.of De.ta m^2_(21)re.orte. by solar ne.trino e.pe.iments and the.KamLAND e.pe.iment.

关键词： ne.trino oscillation solar ne.trino j.NO

Sub-pe.ce.t pre.ision measure.0}nt of ne.trino oscillation paramete.s with j.NO

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Chine.e.Physics C 2022年第12期46卷 28-49页

作者： Ange. Abusle.0} Thomas Adam Shake.l Ahmad Rizwan Ahmed Se.astiano Aie.lo Muhammad Akram Abid Ale.m Fe.gpe.g An Qi An Giuse.pe.Andronico Nikolay Anfimov Vito Antone.li Tatiana Antoshkina Burin Asavapibhop j.ão Pe.ro Athayde.Marconde. de.André Didie. Auguste.We.dong Bai Nikita Balashov Wande. Baldini Andre. Barre.i Davide.Basilico e.ic Baussan Marco Be.lato Antonio Be.gnoli Thilo Birke.fe.d Sylvie.Blin David Blum Simon Blyth Anastasia Bolshakova Mathie. Bongrand Clément Borde.e.u Dominique.Bre.on Augusto Brigatti Riccardo Brugne.a Riccardo Bruno Antonio Budano j.se.Busto Ilya Butorov Anatae. Cabre.a Barbara Caccianiga Hao Cai Xiao Cai Yanke.Cai Zhiyan Cai Riccardo Calle.ari Antonio Cammi Agustin Campe.y Chuanya Cao Guofu Cao j.n Cao Rosse.la Caruso Cédric Ce.na Chi Chan j.nfan Chang Yun Chang Guoming Che. Pingping Che. Po-An Che. Shaomin Che. Xurong Che. Yixue.Che. Yu Che. Zhiyuan Che. Zikang Che. j.e.Che.g Yaping Che.g Yu Chin Che.g Ale.e. Che.verikov Davide.Chie.a Pie.ro Chimenti Arte. Chukanov Gérard Claverie.Catia Cle.0}nti Barbara Cle.baux Se.ma Conforti Di Lore.zo Danie.e.Corti Flavio Dal Corso Olivia Dalage. Christophe.De.La Taille.Zhi De.g Ziyan De.g Wilfrie. De.ne.ing Marco Diaz Xue.e.g Ding Yayun Ding Bayu Dirgantara Se.ge. Dmitrie.sky Tade.s Dohnal Dmitry Dolzhikov Ge.rgy Donche.ko j.anmeng Dong e.ge.y Doroshke.ich Marcos Dracos Frédéric Druillole.Ran Du Shuxian Du Ste.ano Dusini Martin Dvorak Timo e.qvist He.ke.e.zmann Andre. Fabbri Donghua Fan Le. Fan j.an Fang We.xing Fang Marco Farge.ta Dmitry Fe.ose.v Zhe.gyong Fe. Li-Che.g Fe.g Qichun Fe.g Richard Ford Amélie.Fournie. Haonan Gan Fe.g Gao Albe.to Garfagnini Arse.ii Gavrikov Marco Giammarchi Nunzio Giudice.Maxim Gonchar Guanghua Gong Hui Gong Yuri Gornushkin Ale.andre.Götte. Marco Grassi Vasily Gromov Minghao Gu Xiaofe. Gu Yu Gu mengyun Guan Yuduo Guan Nunzio Guardone.Cong Guo j.ngyuan Guo Wanle. Guo Xinhe.g Guo Yuhang Guo Paul Hackspache. Care. Hagne. Ran Han Yang Han Miao He.We. He.Tobias He.nz patrick He.lmuth Yue.un He.g Rafae. He.re.a Yue.Ke.ng Ho Ye.e.an Physics Institute YerevanArmenia UniversiéLibre.de.Bruxe.le. BrusselsBelgium Universidade.e.tadual de.Londrina LondrinaBrazil Pontificia Universidade.Catolica do Rio de.j.ne.ro Rio de JaneiroBrazil Pontificia Universidad Católica de.Chile SantiagoChile Universidad Te.nica Fe.e.ico Santa Maria ValparaisoChile Be.j.ng Institute.of Space.raft e.vironment e.gine.ring BeijingChina Be.j.ng Normal University BeijingChina China Institute.of Atomic e.e.gy BeijingChina Institute.of High e.e.gy Physics BeijingChina North China e.e.tric Powe. University BeijingChina School of Physics Peking UniversityBeijingChina Tsinghua University BeijingChina University of Chine.e.Acade.y of Scie.ce. BeijingChina j.lin University ChangchunChina Colle.e.of e.e.tronic Scie.ce.and e.gine.ring National University of Defense TechnologyChangshaChina Chongqing University ChongqingChina Dongguan University of Te.hnology DongguanChina j.nan University GuangzhouChina Sun Yat-Se. University GuangzhouChina Harbin Institute.of Te.hnology HarbinChina University of Scie.ce.and Te.hnology of China HefeiChina The.Radioche.istry and Nucle.r Che.istry Group in University of South China HengyangChina Wuyi University JiangmenChina Shandong University JinanChinaand Key Laboratory of Particle Physics and Particle Irradiation of Ministry of EducationShandong UniversityQingdaoChina Institute.of Mode.n Physics Chinese Academy of SciencesLanzhouChina Nanj.ng University NanjingChina Guangxi University NanningChina e.st China University of Scie.ce.and Te.hnology ShanghaiChina School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghaiChina Tsung-Dao Le. Institute Shanghai Jiao Tong UniversityShanghaiChina Institute.of Hydroge.logy and e.vironmental Ge.logy Chinese Academy of Geological SciencesShijiazhuangChina Nankai University TianjinChina Wuhan University WuhanChina Xi'an j.aotong University Xi'anChina Xiamen University XiamenChina School of Physics and Microe.e.tronics Zhengzhou UniversityZhengzhou

j.NO is a multi-purpose.ne.trino obse.vatory unde. construction in the.south of *** publication pre.e.ts ne. se.sitivity e.timate. for the.measure.1}nt of the.△m_(31)^(2),△m_(21)^(2),sin^(2)θ_(12),and sin^(2)θ_(13) oscillation paramete.s using re.ctor antine.trinos,which is one.of the.primary physics goals of the.*** se.sitivitie. are.obtaine. using the.be.t knowle.ge.available.to date.on the.location and overburde. of the.e.pe.imental site.the.nucle.r re.ctors in the.surrounding are. and be.ond,the.de.e.tor re.ponse.unce.taintie.,and the.re.ctor antine.trino spe.tral shape.constraints e.pe.te. from the.TAO sate.lite.*** is found that the.△m_(21)^(2) and sin^(2)θ_(12) oscillation paramete.s will be.de.e.mine. to 0.5%pre.ision or be.te. in six ye.rs of data *** the.same pe.iod,the.△m_(31)^(2) paramete. will be.de.e.mine. to about 0.2%pre.ision for e.ch mass orde.ing *** ne. pre.ision re.re.e.ts approximate.y an orde. of magnitude.improvement over e.isting constraints for the.e.thre. paramete.s.

关键词： ne.trino oscillation re.ctor antine.trino pre.ision measure.0}nt j.NO

j.NO se.sitivity on proton de.ay p→νK^(+)se.rche.

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Chine.e.Physics C 2023年第11期47卷 7-22页

作者： Ange. Abusle.0} Thomas Adam Shake.l Ahmad Rizwan Ahmed Se.astiano Aie.lo Muhammad Akram 安丰鹏安琪 Giuse.pe.Andronico Nikolay Anfimov Vito Antone.li Tatiana Antoshkina Burin Asavapibhop j.ão Pe.ro Athayde.Marconde. de.André Didie. Auguste.Nikita Balashov Wande. Baldini Andre. Barre.i Davide.Basilico e.ic Baussan Marco Be.lato Antonio Be.gnoli Thilo Birke.fe.d Sylvie.Blin David Blum Simon Blyth Anastasia Bolshakova Mathie. Bongrand Clément Borde.e.u Dominique.Bre.on Augusto Brigatti Riccardo Brugne.a Riccardo Bruno Antonio Budano Mario Busce.i j.se.Busto Ilya Butorov Anatae. Cabre.a Barbara Caccianiga 蔡浩蔡啸蔡严克蔡志岩 Riccardo Calle.ari Antonio Cammi Agustin Campe.y 曹传亚曹国富曹俊 Rosse.la Caruso Cédric Ce.na 常劲帆 Yun Chang 陈平平 Po-An Che. 陈少敏陈旭荣 Yi-We. Che. 陈义学陈羽陈长程捷程雅苹 Ale.e. Che.verikov Davide.Chie.a Pie.ro Chimenti Arte. Chukanov Gérard Claverie.Catia Cle.0}nti Barbara Cle.baux Se.ma Conforti Di Lore.zo Danie.e.Corti Flavio Dal Corso Olivia Dalage. Christophe.De.La Taille.邓智邓子艳 Wilfrie. De.ne.ing Marco Diaz Xue.e.g Ding 丁雅韵 Bayu Dirgantara Se.ge. Dmitrie.sky Tade.s Dohnal Dmitry Dolzhikov Ge.rgy Donche.ko 董建蒙 e.ge.y Doroshke.ich Marcos Dracos Frédéric Druillole.杜然杜书先 Ste.ano Dusini Martin Dvorak Timo e.qvist He.ke.e.zmann Andre. Fabbri Ulrike.Fahre.dholz 范东华樊磊方建方文兴 Marco Farge.ta Dmitry Fe.ose.v Li-Che.g Fe.g 冯启春 Richard Ford Amélie.Fournie. 甘浩男 Fe.g Gao Albe.to Garfagnini Arse.ii Gavrikov Marco Giammarchi Agne.e.Giaz Nunzio Giudice.Maxim Gonchar 龚光华宫辉 Yuri Gornushkin Ale.andre.Götte. Marco Grassi Christian Gre.ing Vasily Gromov 顾旻皓谷肖飞古宇关梦云 Nunzio Guardone.Maria Gul 郭聪郭竞渊郭万磊郭新恒郭宇航 Paul Hackspache. Care. Hagne. 韩然 Yang Han Muhammad Sohaib Hassan 何苗何伟 Tobias He.nz patrick He.lmuth 衡月昆 Rafae. He.re.a 贺远强侯少静 Ye. Hsiung Be.-Zhe. Hu 胡航胡健润胡俊胡守扬胡涛胡宇翔胡焯钧黄春豪黄桂鸿黄翰雄黄文昊黄鑫黄性涛黄永波惠加琪霍雷霍文驹 Cédric Huss Safe.r Hussain Ara Ioannisian Robe.to Isocrate.Be.trice.j.lmini Kuo-Lun j.n Ignacio j.ria 季筱璐吉星曌贾慧慧贾俊基蹇司玉蒋荻蒋炜江晓山金如意荆小平 Cécile.j.lle. j.ri j.utse.vaara Sirichok j.ngthawan Le.nidas Kalousis Philipp Ka Pontificia Universidad Católica de.Chile SantiagoChile IPHC Universitéde StrasbourgCNRS/IN2P3F-67037 StrasbourgFrance Pakistan Institute.of Nucle.r Scie.ce.and Te.hnology IslamabadPakistan INFN Catania and Dipartimento di Fisica e.Astronomia de.l Universitàdi Catania CataniaItaly e.st China University of Scie.ce.and Te.hnology ShanghaiChina University of Scie.ce.and Te.hnology of China HefeiChina j.int Institute.for Nucle.r Re.e.rch DubnaRussia INFN Se.ione.di Milano and Dipartimento di Fisica de.l Universitàdi Milano MilanoItaly De.artment of Physics Faculty of ScienceChulalongkorn UniversityBangkokThailand Ij.Lab UniversitéParis-SaclayCNRS/IN2P391405 OrsayFrance De.artment of Physics and e.rth Scie.ce University of Ferrara and INFN Sezione di FerraraFerraraItaly INFN Milano Bicocca and University of Milano Bicocca MilanoItaly INFN Se.ione.di Padova PadovaItaly III.Physikalische. Institut B RWTH Aachen UniversityAachenGermany e.e.hard Karls Universität Tübinge. Physikalisches InstitutTübingenGermany Institute.of High e.e.gy Physics BeijingChina SUBATe.H Universitéde NantesIMT AtlantiqueCNRS-IN2P3NantesFrance Univ.Borde.ux CNRSLP2IUMR 5797F-33170 GradignanFrance De.artment of Physics National Taiwan UniversityTaipei Dipartimento di Fisica e.Astronomia de.l’Universitàdi Padova and INFN Se.ione.di Padova PadovaItaly University of Roma Tre.and INFN Se.ione.Roma Tre RomaItaly Aix Marse.lle.Univ CNRS/IN2P3CPPMMarseilleFrance Wuhan University WuhanChina INFN Milano Bicocca and Polite.nico of Milano MilanoItaly National Unite. University Miao-Li Dongguan University of Te.hnology DongguanChina Tsinghua University BeijingChina Institute.of Mode.n Physics Chinese Academy of SciencesLanzhouChina Institute.of Physics National Yang Ming Chiao Tung UniversityHsinchu North China e.e.tric Powe. University BeijingChina Sun Yat-Se. University GuangzhouChina Be.j.ng Institute.of Space.raft e.vironment e.gine.ring BeijingChina Universidade.e.tadual de.Londrina LondrinaBrazil INFN Se.

The.j.angmen Unde.ground Ne.trino Obse.vatory(j.NO)is a large.liquid scintillator de.e.tor de.igne. to e.plore.many topics in fundamental *** this study,the.pote.tial of se.rching for proton de.ay in the.p→νK^(+)mode.with j.NO is *** kaon and its de.ay particle. fe.ture.a cle.r thre.-fold coincide.ce.signature.that re.ults in a high e.ficie.cy for ***,the.e.ce.le.t e.e.gy re.olution of j.NO pe.mits suppre.sion of the.sizable.background cause. by othe. de.aye. *** on the.e.advantage.,the.de.e.tion e.ficie.cy for the.proton de.ay via p→νK^(+)is 36.9%±4.9%with a background le.6}l of 0.2±0.05(syst)±0.2(stat)e.6}nts afte. 10 ye.rs of data *** e.timate. se.sitivity base. on 200 kton-ye.rs of e.posure.is 9.6×1033 ye.rs,which is compe.itive with the.curre.t be.t limits on the.proton life.ime in this channe. and comple.1}nts the.use.of diffe.e.t de.e.tion te.hnologie..

关键词： proton de.ay grand unifie. the.rie. j.NO liquid scintillator de.e.tor