약하게 상호작용하는 무거운 입자 (Korean Wikipedia)

Analysis of information sources in references of the Wikipedia article "약하게 상호작용하는 무거운 입자" in Korean language version.

refsWebsite

Global rank Korean rank

10arxiv.org

69^th place

54^th place

8web.archive.org

1^st place

4doi.org

2^nd place

3^rd place

3harvard.edu

18^th place

27^th place

2stanford.edu

179^th place

146^th place

1archive.org

6^th place

18^th place

1mpg.de

1,624^th place

786^th place

1startribune.com

914^th place

5,533^rd place

1berkeley.edu

580^th place

476^th place

1sciencemag.org

857^th place

295^th place

1nature.com

234^th place

148^th place

1aps.org

1,503^rd place

540^th place

1luxdarkmatter.org

low place

1infn.it

low place

1sites.google.com

626^th place

596^th place

1imperial.ac.uk

7,025^th place

3,399^th place

aps.org (Global: 1,503^rd place; Korean: 540^th place)

prola.aps.org

A. Drukier, K. Freese, and D. Spergel, Detecting Cold Dark Matter Candidates^{[깨진 링크(과거 내용 찾기)]}, Phys.Rev.D33:3495-3508 (1986).

archive.org (Global: 6^th place; Korean: 18^th place)

Griest, Kim (1991). “Galactic Microlensing as a Method of Detecting Massive Compact Halo Objects”. 《The Astrophysical Journal》 366: 412–421. Bibcode:1991ApJ...366..412G. doi:10.1086/169575.

arxiv.org (Global: 69^th place; Korean: 54^th place)

arxiv.org

T. Daylan, et al., The Characterization of the Gamma-Ray Signal from the Central Milky Way: A Compelling Case for Annihilating Dark Matter
H.V. Klapdor-Kleingrothaus, Double Beta Decay and Dark Matter Search - Window to New Physics now, and in future (GENIUS), 4 Feb 1998
M. Kamionkowski, WIMP and Axion Dark Matter, 24 Oct 1997
V. Zacek, Dark Matter Proc. of the 2007 Lake Louise Winter Institute, March 2007
K. Griest, The Search for Dark Matter: WIMPs and MACHOs, 13 Mar 1993
C. Conroy, R. H. Wechsler, A. V. Kravtsov, Modeling Luminosity-Dependent Galaxy Clustering Through Cosmic Time, 21 Feb 2006.
F. Ferrer, L. Krauss, and S. Profumo, Indirect detection of light neutralino dark matter in the NMSSM. Phys.Rev. D74 (2006) 115007
Merritt, D.; Bertone, G. (2005). “Dark Matter Dynamics and Indirect Detection”. 《Modern Physics Letters A》 20 (14): 1021–1036. arXiv:astro-ph/0504422. Bibcode:2005MPLA...20.1021B. doi:10.1142/S0217732305017391.
CoGeNT collaboration (C. E. Aalseth (2011). “Results from a Search for Light-Mass Dark Matter with a P-type Point Contact Germanium Detector”. 《Physical Review Letters》 106 (13). arXiv:1002.4703. Bibcode:2011PhRvL.106m1301A. doi:10.1103/PhysRevLett.106.131301.

xxx.arxiv.org

N. Fornengo, Status and perspectives of indirect and direct dark matter searches^{[깨진 링크(과거 내용 찾기)]}. 36th COSPAR Scientific Assembly, Beijing, China, 16–23 July 2006

berkeley.edu (Global: 580^th place; Korean: 476^th place)

cdms.berkeley.edu

CDMS Collaboration. “Results from the Final Exposure of the CDMS II Experiment” (PDF). 2009년 12월 29일에 원본 문서 (PDF)에서 보존된 문서. 2014년 4월 25일에 확인함. . See also a non-technical summary: CDMS Collaboration. “Latest Results in the Search for Dark Matter” (PDF). 2010년 6월 18일에 원본 문서 (PDF)에서 보존된 문서. 2009년 12월 21일에 확인함.

doi.org (Global: 2^nd place; Korean: 3^rd place)

dx.doi.org

Griest, Kim (1991). “Galactic Microlensing as a Method of Detecting Massive Compact Halo Objects”. 《The Astrophysical Journal》 366: 412–421. Bibcode:1991ApJ...366..412G. doi:10.1086/169575.
Merritt, D.; Bertone, G. (2005). “Dark Matter Dynamics and Indirect Detection”. 《Modern Physics Letters A》 20 (14): 1021–1036. arXiv:astro-ph/0504422. Bibcode:2005MPLA...20.1021B. doi:10.1142/S0217732305017391.
The CDMS II Collaboration (2010). “Dark Matter Search Results from the CDMS II Experiment”. Science. doi:10.1126/science.1186112.
CoGeNT collaboration (C. E. Aalseth (2011). “Results from a Search for Light-Mass Dark Matter with a P-type Point Contact Germanium Detector”. 《Physical Review Letters》 106 (13). arXiv:1002.4703. Bibcode:2011PhRvL.106m1301A. doi:10.1103/PhysRevLett.106.131301.

harvard.edu (Global: 18^th place; Korean: 27^th place)

adsabs.harvard.edu

Griest, Kim (1991). “Galactic Microlensing as a Method of Detecting Massive Compact Halo Objects”. 《The Astrophysical Journal》 366: 412–421. Bibcode:1991ApJ...366..412G. doi:10.1086/169575.
Merritt, D.; Bertone, G. (2005). “Dark Matter Dynamics and Indirect Detection”. 《Modern Physics Letters A》 20 (14): 1021–1036. arXiv:astro-ph/0504422. Bibcode:2005MPLA...20.1021B. doi:10.1142/S0217732305017391.
CoGeNT collaboration (C. E. Aalseth (2011). “Results from a Search for Light-Mass Dark Matter with a P-type Point Contact Germanium Detector”. 《Physical Review Letters》 106 (13). arXiv:1002.4703. Bibcode:2011PhRvL.106m1301A. doi:10.1103/PhysRevLett.106.131301.

imperial.ac.uk (Global: 7,025^th place; Korean: 3,399^th place)

hep.ph.imperial.ac.uk

http://www.hep.ph.imperial.ac.uk/ZEPLIN-III-Project/

infn.it (Global: low place; Korean: low place)

darkside.lngs.infn.it

“보관된 사본”. 2012년 11월 3일에 원본 문서에서 보존된 문서. 2014년 4월 25일에 확인함.

luxdarkmatter.org (Global: low place; Korean: low place)

“보관된 사본”. 2021년 1월 15일에 원본 문서에서 보존된 문서. 2014년 4월 25일에 확인함.

mpg.de (Global: 1,624^th place; Korean: 786^th place)

mpa-garching.mpg.de

The Millennium Simulation Project , Introduction: The Millennium Simulation The Millennium Run used more than 10 billion particles to trace the evolution of the matter distribution in a cubic region of the Universe over 2 billion light-years on a side.

nature.com (Global: 234^th place; Korean: 148^th place)

Eric Hand (2010년 2월 26일). “A CoGeNT result in the hunt for dark matter”. Nature News.

sciencemag.org (Global: 857^th place; Korean: 295^th place)

The CDMS II Collaboration (2010). “Dark Matter Search Results from the CDMS II Experiment”. Science. doi:10.1126/science.1186112.

sites.google.com (Global: 626^th place; Korean: 596^th place)

http://sites.google.com/site/dm2011simple/

stanford.edu (Global: 179^th place; Korean: 146^th place)

slac.stanford.edu

K. Freese, Can Scalar Neutrinos Or Massive Dirac Neutrinos Be the Missing Mass? ^{[깨진 링크(과거 내용 찾기)]}. Phys.Lett.B167:295 (1986).
K. Freese, J. Frieman, and A. Gould, Signal Modulation in Cold Dark Matter Detection 보관됨 2015-09-24 - 웨이백 머신, Phys.Rev.D37:3388 (1988).

startribune.com (Global: 914^th place; Korean: 5,533^rd place)

“Key to the universe found on the Iron Range?”. 2009년 12월 22일에 원본 문서에서 보존된 문서. 2009년 12월 18일에 확인함.

web.archive.org (Global: 1^st place; Korean: 1^st place)

K. Freese, Can Scalar Neutrinos Or Massive Dirac Neutrinos Be the Missing Mass? ^{[깨진 링크(과거 내용 찾기)]}. Phys.Lett.B167:295 (1986).
N. Fornengo, Status and perspectives of indirect and direct dark matter searches^{[깨진 링크(과거 내용 찾기)]}. 36th COSPAR Scientific Assembly, Beijing, China, 16–23 July 2006
“Key to the universe found on the Iron Range?”. 2009년 12월 22일에 원본 문서에서 보존된 문서. 2009년 12월 18일에 확인함.
CDMS Collaboration. “Results from the Final Exposure of the CDMS II Experiment” (PDF). 2009년 12월 29일에 원본 문서 (PDF)에서 보존된 문서. 2014년 4월 25일에 확인함. . See also a non-technical summary: CDMS Collaboration. “Latest Results in the Search for Dark Matter” (PDF). 2010년 6월 18일에 원본 문서 (PDF)에서 보존된 문서. 2009년 12월 21일에 확인함.
A. Drukier, K. Freese, and D. Spergel, Detecting Cold Dark Matter Candidates^{[깨진 링크(과거 내용 찾기)]}, Phys.Rev.D33:3495-3508 (1986).
K. Freese, J. Frieman, and A. Gould, Signal Modulation in Cold Dark Matter Detection 보관됨 2015-09-24 - 웨이백 머신, Phys.Rev.D37:3388 (1988).
“보관된 사본”. 2021년 1월 15일에 원본 문서에서 보존된 문서. 2014년 4월 25일에 확인함.
“보관된 사본”. 2012년 11월 3일에 원본 문서에서 보존된 문서. 2014년 4월 25일에 확인함.

약하게 상호작용하는 무거운 입자 (Korean Wikipedia)

aps.org (Global: 1,503rd place; Korean: 540th place)

prola.aps.org

archive.org (Global: 6th place; Korean: 18th place)

arxiv.org (Global: 69th place; Korean: 54th place)

arxiv.org

xxx.arxiv.org

berkeley.edu (Global: 580th place; Korean: 476th place)

cdms.berkeley.edu

doi.org (Global: 2nd place; Korean: 3rd place)