Pith. sign in

REVIEW 4 cited by

Dark Matter Results from First 98.7-day Data of PandaX-II Experiment

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1607.07400 v3 pith:5X2R3IGJ submitted 2016-07-25 hep-ex physics.ins-det

PandaX-II Collaboration: Andi Tan , Mengjiao Xiao , Xiangyi Cui , Xun Chen , Yunhua Chen , Deqing Fang , Changbo Fu , Karl Giboni
show 44 more authors
Franco Giuliani Haowei Gong Shouyang Hu Xingtao Huang Xiangdong Ji Yonglin Ju Siao Lei Shaoli Li Xiaomei Li Xinglong Li Hao Liang Qing Lin Huaxuan Liu Jianglai Liu Wolfgang Lorenzon Yugang Ma Yajun Mao Kaixuan Ni Xiangxiang Ren Michael Schubnell Manbin Shen Fang Shi Hongwei Wang Jiming Wang Meng Wang Qiuhong Wang Siguang Wang Xuming Wang Zhou Wang Shiyong Wu Xiang Xiao Pengwei Xie Binbin Yan Yong Yang Jianfeng Yue Xionghui Zeng Hongguang Zhang Hua Zhang Huanqiao Zhang Tao Zhang Li Zhao Jing Zhou Ning Zhou Xiaopeng Zhou
This is my paper · ORCID
classification hep-exphysics.ins-det
keywords darkmatterdatawimpfirstlimitmasspandax-ii
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

We report the WIMP dark matter search results using the first physics-run data of the PandaX-II 500 kg liquid xenon dual-phase time-projection chamber, operating at the China JinPing Underground Laboratory. No dark matter candidate is identified above background. In combination with the data set during the commissioning run, with a total exposure of 3.3$\times10^4$ kg-day,the most stringent limit to the spin-independent interaction between the ordinary and WIMP dark matter is set for a range of dark matter mass between 3.5 and 1000 GeV/c$^2$. The best upper limit on the scattering cross section is found $2.5\times 10^{-46}$ cm$^2$ for the WIMP mass 40 GeV/c$^2$ at 90% confidence level.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Axion-like Particle Search with a Light-Shining-Through-Walls Setup at a $\gamma$-$\gamma$ Collider

    hep-ph 2025-12 conditional novelty 6.0 of 10

    A light-shining-through-walls search using a gamma-gamma collider's inverse-Compton photon beam could reach g_aγγ ≈ 3.8e-5 GeV^-1 for m_a < 0.1 eV.

  2. Diversity of Fuzzy Dark Matter Solitons

    hep-ph 2024-11 conditional novelty 6.0 of 10

    Environmental effects, especially a central black hole and baryonic matter, can substantially alter fuzzy dark matter soliton profiles, while the soliton's own gravitomagnetic field is negligible.

  3. Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos

    hep-ph 2019-07 unverdicted novelty 5.0 of 10

    The thesis presents a new 3-to-2 freezeout mechanism, bound-state effects on searches, a new axion interferometric search, reionization assessments, 21-cm constraints, and the DarkHistory code for ionization and therm...

  4. Dark matter from axion and small neutrino mass

    hep-ph 2024-12 conditional novelty 4.0 of 10

    A KSVZ-like model with a fermion dark matter candidate produced by UV freeze-in through the axion portal is shown to have viable parameter space at TeV mass and axion decay constant near 10^10 to 10^11 GeV.

Pith tools