Dark matter direct search sensitivity of the PandaX-4T experiment
The PandaX-4T experiment, a 4-ton scale dark matter direct detection experiment, is being planned at the China Jinping Un- derground Laboratory. In this paper we present a simulation study of the expected background in this experiment. In a 2.8-ton fiducial mass and the signal region between 1–10 ke...
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| Veröffentlicht in: | Science China. Physics, mechanics & astronomy mechanics & astronomy, 2019-03, Vol.62 (3), p.31011, Article 31011 |
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| creator | Zhang, HongGuang Abdukerim, Abdusalam Chen, Wei Chen, Xun Chen, YunHua Cui, XiangYi Dong, BinBin Fang, DeQing Fu, ChangBo Giboni, Karl Giuliani, Franco Gu, LinHui Guo, XuYuan Guo, ZhiFan Han, Ke He, ChangDa He, ShengMing Huang, Di Huang, XingTao Huang, Zhou Ji, Peng Ji, XiangDong Ju, YongLin Li, ShaoLi Li, Yao Lin, Heng Liu, HuaXuan Liu, JiangLai Ma, YuGang Mao, YaJun Ni, KaiXiang Ning, JinHua Ren, XiangXiang Shi, Fang Tan, AnDi Wang, AnQing Wang, Cheng Wang, HongWei Wang, Meng Wang, QiuHong Wang, SiGuang Wang, XiuLi Wang, XuMing Wang, Zhou Wu, MengMeng Wu, ShiYong Xia, JingKai Xiao, MengJiao Xie, PengWei Yan, BinBin Yang, JiJun Yang, Yong Yu, ChunXu Yuan, JuMin Yue, JianFeng Zhang, Dan Zhang, Tao Zhao, Li Zheng, QiBin Zhou, JiFang Zhou, Ning Zhou, XiaoPeng |
| description | The PandaX-4T experiment, a 4-ton scale dark matter direct detection experiment, is being planned at the China Jinping Un- derground Laboratory. In this paper we present a simulation study of the expected background in this experiment. In a 2.8-ton fiducial mass and the signal region between 1–10 keV electron equivalent energy, the total electron recoil background is found to be 4:9 × 10
−5
kg
−1
d
−1
keV
−1
. The nuclear recoil background in the same region is 2:8 × 10
−7
kg
−1
d
−1
keV
−1
. With an exposure of 5.6 ton-years, the sensitivity of PandaX-4T could reach a minimum spin-independent dark matter-nucleon cross section of 6 × 10
−48
cm
2
at a dark matter mass of 40 GeV/
c
2
. |
| doi_str_mv | 10.1007/s11433-018-9259-0 |
| format | Article |
| fullrecord | <record><control><sourceid>gale_proqu</sourceid><recordid>TN_cdi_proquest_journals_2918585602</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><galeid>A727506225</galeid><sourcerecordid>A727506225</sourcerecordid><originalsourceid>FETCH-LOGICAL-c421t-d898f09a7fb6111fbb504d3a6241e5653f967674e6403395d6ba1b06d446330d3</originalsourceid><addsrcrecordid>eNp1kEtLAzEUhYMoWGp_gLsB16l5Z7Is9QkFXVRwFzKTpE1tZ2qSiv33pozgymRxw-V8N-ceAK4xmmKE5G3CmFEKEa6hIlxBdAZGuBYKYkXkeXkLyaCkrL4Ek5Q2qByqEJNsBGZ3Jn5UO5Ozi5UN0bW5Ss7Edl1Kl0IOXyEfq95Xee2qV9NZ8w7ZsnLfexfDznX5Clx4s01u8lvH4O3hfjl_gouXx-f5bAFbRnCGtla1R8pI3wiMsW8ajpilRhCGHReceiVk8ekEQ5QqbkVjcIOEZUxQiiwdg5th7j72nweXst70h9iVLzVRuOY1F4gU1XRQrczW6dD5PkfTlmvdLrR953wo_ZkkkiNBCC8AHoA29ilF5_W-7GXiUWOkT-nqIV1d0tWndDUqDBmYVLTdysU_K_9DP54EefA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2918585602</pqid></control><display><type>article</type><title>Dark matter direct search sensitivity of the PandaX-4T experiment</title><source>Springer Nature - Complete Springer Journals</source><source>Alma/SFX Local Collection</source><creator>Zhang, HongGuang ; Abdukerim, Abdusalam ; Chen, Wei ; Chen, Xun ; Chen, YunHua ; Cui, XiangYi ; Dong, BinBin ; Fang, DeQing ; Fu, ChangBo ; Giboni, Karl ; Giuliani, Franco ; Gu, LinHui ; Guo, XuYuan ; Guo, ZhiFan ; Han, Ke ; He, ChangDa ; He, ShengMing ; Huang, Di ; Huang, XingTao ; Huang, Zhou ; Ji, Peng ; Ji, XiangDong ; Ju, YongLin ; Li, ShaoLi ; Li, Yao ; Lin, Heng ; Liu, HuaXuan ; Liu, JiangLai ; Ma, YuGang ; Mao, YaJun ; Ni, KaiXiang ; Ning, JinHua ; Ren, XiangXiang ; Shi, Fang ; Tan, AnDi ; Wang, AnQing ; Wang, Cheng ; Wang, HongWei ; Wang, Meng ; Wang, QiuHong ; Wang, SiGuang ; Wang, XiuLi ; Wang, XuMing ; Wang, Zhou ; Wu, MengMeng ; Wu, ShiYong ; Xia, JingKai ; Xiao, MengJiao ; Xie, PengWei ; Yan, BinBin ; Yang, JiJun ; Yang, Yong ; Yu, ChunXu ; Yuan, JuMin ; Yue, JianFeng ; Zhang, Dan ; Zhang, Tao ; Zhao, Li ; Zheng, QiBin ; Zhou, JiFang ; Zhou, Ning ; Zhou, XiaoPeng</creator><creatorcontrib>Zhang, HongGuang ; Abdukerim, Abdusalam ; Chen, Wei ; Chen, Xun ; Chen, YunHua ; Cui, XiangYi ; Dong, BinBin ; Fang, DeQing ; Fu, ChangBo ; Giboni, Karl ; Giuliani, Franco ; Gu, LinHui ; Guo, XuYuan ; Guo, ZhiFan ; Han, Ke ; He, ChangDa ; He, ShengMing ; Huang, Di ; Huang, XingTao ; Huang, Zhou ; Ji, Peng ; Ji, XiangDong ; Ju, YongLin ; Li, ShaoLi ; Li, Yao ; Lin, Heng ; Liu, HuaXuan ; Liu, JiangLai ; Ma, YuGang ; Mao, YaJun ; Ni, KaiXiang ; Ning, JinHua ; Ren, XiangXiang ; Shi, Fang ; Tan, AnDi ; Wang, AnQing ; Wang, Cheng ; Wang, HongWei ; Wang, Meng ; Wang, QiuHong ; Wang, SiGuang ; Wang, XiuLi ; Wang, XuMing ; Wang, Zhou ; Wu, MengMeng ; Wu, ShiYong ; Xia, JingKai ; Xiao, MengJiao ; Xie, PengWei ; Yan, BinBin ; Yang, JiJun ; Yang, Yong ; Yu, ChunXu ; Yuan, JuMin ; Yue, JianFeng ; Zhang, Dan ; Zhang, Tao ; Zhao, Li ; Zheng, QiBin ; Zhou, JiFang ; Zhou, Ning ; Zhou, XiaoPeng</creatorcontrib><description>The PandaX-4T experiment, a 4-ton scale dark matter direct detection experiment, is being planned at the China Jinping Un- derground Laboratory. In this paper we present a simulation study of the expected background in this experiment. In a 2.8-ton fiducial mass and the signal region between 1–10 keV electron equivalent energy, the total electron recoil background is found to be 4:9 × 10
−5
kg
−1
d
−1
keV
−1
. The nuclear recoil background in the same region is 2:8 × 10
−7
kg
−1
d
−1
keV
−1
. With an exposure of 5.6 ton-years, the sensitivity of PandaX-4T could reach a minimum spin-independent dark matter-nucleon cross section of 6 × 10
−48
cm
2
at a dark matter mass of 40 GeV/
c
2
.</description><identifier>ISSN: 1674-7348</identifier><identifier>EISSN: 1869-1927</identifier><identifier>DOI: 10.1007/s11433-018-9259-0</identifier><language>eng</language><publisher>Beijing: Science China Press</publisher><subject>Astronomy ; Classical and Continuum Physics ; Cosmic rays ; Cosmology ; Dark matter ; Experiments ; Laboratories ; Observations and Techniques ; Particle physics ; Physics ; Physics and Astronomy ; Recoil ; Sensitivity ; Sensors</subject><ispartof>Science China. Physics, mechanics & astronomy, 2019-03, Vol.62 (3), p.31011, Article 31011</ispartof><rights>Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2018</rights><rights>COPYRIGHT 2019 Springer</rights><rights>Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2018.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c421t-d898f09a7fb6111fbb504d3a6241e5653f967674e6403395d6ba1b06d446330d3</citedby><cites>FETCH-LOGICAL-c421t-d898f09a7fb6111fbb504d3a6241e5653f967674e6403395d6ba1b06d446330d3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11433-018-9259-0$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11433-018-9259-0$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,777,781,27905,27906,41469,42538,51300</link.rule.ids></links><search><creatorcontrib>Zhang, HongGuang</creatorcontrib><creatorcontrib>Abdukerim, Abdusalam</creatorcontrib><creatorcontrib>Chen, Wei</creatorcontrib><creatorcontrib>Chen, Xun</creatorcontrib><creatorcontrib>Chen, YunHua</creatorcontrib><creatorcontrib>Cui, XiangYi</creatorcontrib><creatorcontrib>Dong, BinBin</creatorcontrib><creatorcontrib>Fang, DeQing</creatorcontrib><creatorcontrib>Fu, ChangBo</creatorcontrib><creatorcontrib>Giboni, Karl</creatorcontrib><creatorcontrib>Giuliani, Franco</creatorcontrib><creatorcontrib>Gu, LinHui</creatorcontrib><creatorcontrib>Guo, XuYuan</creatorcontrib><creatorcontrib>Guo, ZhiFan</creatorcontrib><creatorcontrib>Han, Ke</creatorcontrib><creatorcontrib>He, ChangDa</creatorcontrib><creatorcontrib>He, ShengMing</creatorcontrib><creatorcontrib>Huang, Di</creatorcontrib><creatorcontrib>Huang, XingTao</creatorcontrib><creatorcontrib>Huang, Zhou</creatorcontrib><creatorcontrib>Ji, Peng</creatorcontrib><creatorcontrib>Ji, XiangDong</creatorcontrib><creatorcontrib>Ju, YongLin</creatorcontrib><creatorcontrib>Li, ShaoLi</creatorcontrib><creatorcontrib>Li, Yao</creatorcontrib><creatorcontrib>Lin, Heng</creatorcontrib><creatorcontrib>Liu, HuaXuan</creatorcontrib><creatorcontrib>Liu, JiangLai</creatorcontrib><creatorcontrib>Ma, YuGang</creatorcontrib><creatorcontrib>Mao, YaJun</creatorcontrib><creatorcontrib>Ni, KaiXiang</creatorcontrib><creatorcontrib>Ning, JinHua</creatorcontrib><creatorcontrib>Ren, XiangXiang</creatorcontrib><creatorcontrib>Shi, Fang</creatorcontrib><creatorcontrib>Tan, AnDi</creatorcontrib><creatorcontrib>Wang, AnQing</creatorcontrib><creatorcontrib>Wang, Cheng</creatorcontrib><creatorcontrib>Wang, HongWei</creatorcontrib><creatorcontrib>Wang, Meng</creatorcontrib><creatorcontrib>Wang, QiuHong</creatorcontrib><creatorcontrib>Wang, SiGuang</creatorcontrib><creatorcontrib>Wang, XiuLi</creatorcontrib><creatorcontrib>Wang, XuMing</creatorcontrib><creatorcontrib>Wang, Zhou</creatorcontrib><creatorcontrib>Wu, MengMeng</creatorcontrib><creatorcontrib>Wu, ShiYong</creatorcontrib><creatorcontrib>Xia, JingKai</creatorcontrib><creatorcontrib>Xiao, MengJiao</creatorcontrib><creatorcontrib>Xie, PengWei</creatorcontrib><creatorcontrib>Yan, BinBin</creatorcontrib><creatorcontrib>Yang, JiJun</creatorcontrib><creatorcontrib>Yang, Yong</creatorcontrib><creatorcontrib>Yu, ChunXu</creatorcontrib><creatorcontrib>Yuan, JuMin</creatorcontrib><creatorcontrib>Yue, JianFeng</creatorcontrib><creatorcontrib>Zhang, Dan</creatorcontrib><creatorcontrib>Zhang, Tao</creatorcontrib><creatorcontrib>Zhao, Li</creatorcontrib><creatorcontrib>Zheng, QiBin</creatorcontrib><creatorcontrib>Zhou, JiFang</creatorcontrib><creatorcontrib>Zhou, Ning</creatorcontrib><creatorcontrib>Zhou, XiaoPeng</creatorcontrib><title>Dark matter direct search sensitivity of the PandaX-4T experiment</title><title>Science China. Physics, mechanics & astronomy</title><addtitle>Sci. China Phys. Mech. Astron</addtitle><description>The PandaX-4T experiment, a 4-ton scale dark matter direct detection experiment, is being planned at the China Jinping Un- derground Laboratory. In this paper we present a simulation study of the expected background in this experiment. In a 2.8-ton fiducial mass and the signal region between 1–10 keV electron equivalent energy, the total electron recoil background is found to be 4:9 × 10
−5
kg
−1
d
−1
keV
−1
. The nuclear recoil background in the same region is 2:8 × 10
−7
kg
−1
d
−1
keV
−1
. With an exposure of 5.6 ton-years, the sensitivity of PandaX-4T could reach a minimum spin-independent dark matter-nucleon cross section of 6 × 10
−48
cm
2
at a dark matter mass of 40 GeV/
c
2
.</description><subject>Astronomy</subject><subject>Classical and Continuum Physics</subject><subject>Cosmic rays</subject><subject>Cosmology</subject><subject>Dark matter</subject><subject>Experiments</subject><subject>Laboratories</subject><subject>Observations and Techniques</subject><subject>Particle physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Recoil</subject><subject>Sensitivity</subject><subject>Sensors</subject><issn>1674-7348</issn><issn>1869-1927</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>AFKRA</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNp1kEtLAzEUhYMoWGp_gLsB16l5Z7Is9QkFXVRwFzKTpE1tZ2qSiv33pozgymRxw-V8N-ceAK4xmmKE5G3CmFEKEa6hIlxBdAZGuBYKYkXkeXkLyaCkrL4Ek5Q2qByqEJNsBGZ3Jn5UO5Ozi5UN0bW5Ss7Edl1Kl0IOXyEfq95Xee2qV9NZ8w7ZsnLfexfDznX5Clx4s01u8lvH4O3hfjl_gouXx-f5bAFbRnCGtla1R8pI3wiMsW8ajpilRhCGHReceiVk8ekEQ5QqbkVjcIOEZUxQiiwdg5th7j72nweXst70h9iVLzVRuOY1F4gU1XRQrczW6dD5PkfTlmvdLrR953wo_ZkkkiNBCC8AHoA29ilF5_W-7GXiUWOkT-nqIV1d0tWndDUqDBmYVLTdysU_K_9DP54EefA</recordid><startdate>20190301</startdate><enddate>20190301</enddate><creator>Zhang, HongGuang</creator><creator>Abdukerim, Abdusalam</creator><creator>Chen, Wei</creator><creator>Chen, Xun</creator><creator>Chen, YunHua</creator><creator>Cui, XiangYi</creator><creator>Dong, BinBin</creator><creator>Fang, DeQing</creator><creator>Fu, ChangBo</creator><creator>Giboni, Karl</creator><creator>Giuliani, Franco</creator><creator>Gu, LinHui</creator><creator>Guo, XuYuan</creator><creator>Guo, ZhiFan</creator><creator>Han, Ke</creator><creator>He, ChangDa</creator><creator>He, ShengMing</creator><creator>Huang, Di</creator><creator>Huang, XingTao</creator><creator>Huang, Zhou</creator><creator>Ji, Peng</creator><creator>Ji, XiangDong</creator><creator>Ju, YongLin</creator><creator>Li, ShaoLi</creator><creator>Li, Yao</creator><creator>Lin, Heng</creator><creator>Liu, HuaXuan</creator><creator>Liu, JiangLai</creator><creator>Ma, YuGang</creator><creator>Mao, YaJun</creator><creator>Ni, KaiXiang</creator><creator>Ning, JinHua</creator><creator>Ren, XiangXiang</creator><creator>Shi, Fang</creator><creator>Tan, AnDi</creator><creator>Wang, AnQing</creator><creator>Wang, 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Liu, HuaXuan ; Liu, JiangLai ; Ma, YuGang ; Mao, YaJun ; Ni, KaiXiang ; Ning, JinHua ; Ren, XiangXiang ; Shi, Fang ; Tan, AnDi ; Wang, AnQing ; Wang, Cheng ; Wang, HongWei ; Wang, Meng ; Wang, QiuHong ; Wang, SiGuang ; Wang, XiuLi ; Wang, XuMing ; Wang, Zhou ; Wu, MengMeng ; Wu, ShiYong ; Xia, JingKai ; Xiao, MengJiao ; Xie, PengWei ; Yan, BinBin ; Yang, JiJun ; Yang, Yong ; Yu, ChunXu ; Yuan, JuMin ; Yue, JianFeng ; Zhang, Dan ; Zhang, Tao ; Zhao, Li ; Zheng, QiBin ; Zhou, JiFang ; Zhou, Ning ; Zhou, XiaoPeng</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c421t-d898f09a7fb6111fbb504d3a6241e5653f967674e6403395d6ba1b06d446330d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Astronomy</topic><topic>Classical and Continuum Physics</topic><topic>Cosmic rays</topic><topic>Cosmology</topic><topic>Dark 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Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>Engineering Collection</collection><jtitle>Science China. Physics, mechanics & astronomy</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zhang, HongGuang</au><au>Abdukerim, Abdusalam</au><au>Chen, Wei</au><au>Chen, Xun</au><au>Chen, YunHua</au><au>Cui, XiangYi</au><au>Dong, BinBin</au><au>Fang, DeQing</au><au>Fu, ChangBo</au><au>Giboni, Karl</au><au>Giuliani, Franco</au><au>Gu, LinHui</au><au>Guo, XuYuan</au><au>Guo, ZhiFan</au><au>Han, Ke</au><au>He, ChangDa</au><au>He, ShengMing</au><au>Huang, Di</au><au>Huang, XingTao</au><au>Huang, Zhou</au><au>Ji, Peng</au><au>Ji, XiangDong</au><au>Ju, YongLin</au><au>Li, ShaoLi</au><au>Li, Yao</au><au>Lin, Heng</au><au>Liu, HuaXuan</au><au>Liu, JiangLai</au><au>Ma, YuGang</au><au>Mao, YaJun</au><au>Ni, KaiXiang</au><au>Ning, JinHua</au><au>Ren, XiangXiang</au><au>Shi, Fang</au><au>Tan, AnDi</au><au>Wang, AnQing</au><au>Wang, Cheng</au><au>Wang, HongWei</au><au>Wang, Meng</au><au>Wang, QiuHong</au><au>Wang, SiGuang</au><au>Wang, XiuLi</au><au>Wang, XuMing</au><au>Wang, Zhou</au><au>Wu, MengMeng</au><au>Wu, ShiYong</au><au>Xia, JingKai</au><au>Xiao, MengJiao</au><au>Xie, PengWei</au><au>Yan, BinBin</au><au>Yang, JiJun</au><au>Yang, Yong</au><au>Yu, ChunXu</au><au>Yuan, JuMin</au><au>Yue, JianFeng</au><au>Zhang, Dan</au><au>Zhang, Tao</au><au>Zhao, Li</au><au>Zheng, QiBin</au><au>Zhou, JiFang</au><au>Zhou, Ning</au><au>Zhou, XiaoPeng</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Dark matter direct search sensitivity of the PandaX-4T experiment</atitle><jtitle>Science China. Physics, mechanics & astronomy</jtitle><stitle>Sci. China Phys. Mech. Astron</stitle><date>2019-03-01</date><risdate>2019</risdate><volume>62</volume><issue>3</issue><spage>31011</spage><pages>31011-</pages><artnum>31011</artnum><issn>1674-7348</issn><eissn>1869-1927</eissn><abstract>The PandaX-4T experiment, a 4-ton scale dark matter direct detection experiment, is being planned at the China Jinping Un- derground Laboratory. In this paper we present a simulation study of the expected background in this experiment. In a 2.8-ton fiducial mass and the signal region between 1–10 keV electron equivalent energy, the total electron recoil background is found to be 4:9 × 10
−5
kg
−1
d
−1
keV
−1
. The nuclear recoil background in the same region is 2:8 × 10
−7
kg
−1
d
−1
keV
−1
. With an exposure of 5.6 ton-years, the sensitivity of PandaX-4T could reach a minimum spin-independent dark matter-nucleon cross section of 6 × 10
−48
cm
2
at a dark matter mass of 40 GeV/
c
2
.</abstract><cop>Beijing</cop><pub>Science China Press</pub><doi>10.1007/s11433-018-9259-0</doi></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1674-7348 |
| ispartof | Science China. Physics, mechanics & astronomy, 2019-03, Vol.62 (3), p.31011, Article 31011 |
| issn | 1674-7348 1869-1927 |
| language | eng |
| recordid | cdi_proquest_journals_2918585602 |
| source | Springer Nature - Complete Springer Journals; Alma/SFX Local Collection |
| subjects | Astronomy Classical and Continuum Physics Cosmic rays Cosmology Dark matter Experiments Laboratories Observations and Techniques Particle physics Physics Physics and Astronomy Recoil Sensitivity Sensors |
| title | Dark matter direct search sensitivity of the PandaX-4T experiment |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-20T14%3A10%3A07IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-gale_proqu&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Dark%20matter%20direct%20search%20sensitivity%20of%20the%20PandaX-4T%20experiment&rft.jtitle=Science%20China.%20Physics,%20mechanics%20&%20astronomy&rft.au=Zhang,%20HongGuang&rft.date=2019-03-01&rft.volume=62&rft.issue=3&rft.spage=31011&rft.pages=31011-&rft.artnum=31011&rft.issn=1674-7348&rft.eissn=1869-1927&rft_id=info:doi/10.1007/s11433-018-9259-0&rft_dat=%3Cgale_proqu%3EA727506225%3C/gale_proqu%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2918585602&rft_id=info:pmid/&rft_galeid=A727506225&rfr_iscdi=true |