يعرض 1 - 6 نتائج من 6 نتيجة بحث عن '"LAMBDA-CDM COSMOLOGY"', وقت الاستعلام: 0.38s تنقيح النتائج
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    Academic Journal
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    Academic Journal

    المؤلفون: Hou, Jun, Yu, Qingjuan, Lu, Youjun

    المساهمون: Hou, J (reprint author), Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China., Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China., Peking Univ, Sch Phys, Beijing 100871, Peoples R China., Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China.

    المصدر: SCI

    Relation: ASTROPHYSICAL JOURNAL.2014,791,(1).; 766124; http://hdl.handle.net/20.500.11897/147833; WOS:000339657700008

  4. 4
    Academic Journal

    المساهمون: Knebe, A (reprint author), Univ Autonoma Madrid, Fac Ciencias, Dept Fis Teor, Modulo 15, E-28049 Madrid, Spain., Univ Autonoma Madrid, Fac Ciencias, Dept Fis Teor, E-28049 Madrid, Spain., Univ Nottingham, Sch Phys Astron, Nottingham NG7 2RD, England., Univ Oxford, Dept Phys, Oxford OX1 3RH, England., Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94309 USA., Stanford Univ, Dept Phys, Stanford, CA 94305 USA., SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA., Univ Zurich, Inst Theoret Phys, CH-8057 Zurich, Switzerland., Max Planck Inst Astrophys, D-85741 Garching, Germany., Univ Observ Munchen, D-81679 Munich, Germany., Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China., Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England., Leibniz Inst Astrophys Potsdam AIP, D-14482 Potsdam, Germany., Chinese Acad Sci, Grad Sch, Beijing 100039, Peoples R China., Univ Durham, Dept Phys, Inst Computat Cosmol, Durham DH1 3LE, England., New Mexico State Univ, Dept Astron, Las Cruces, NM 88003 USA., Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94610 USA., Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87544 USA., Vanderbilt Univ, Stevenson Ctr 6301, Dept Phys & Astron, Nashville, TN 37235 USA., Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA., UNC, CONICET, CCT Cordoba, Inst Astron Teor & Expt, Cordoba, Argentina., Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA., Univ Trieste, Dept Phys, Astron Unit, I-34131 Trieste, Italy., INAF, Osservatorio Astron Trieste, I-34131 Trieste, Italy., Univ Valencia, Dept Astron & Astrofis, E-46100 Burjassot, Valencia, Spain., Univ Paris Diderot, Observ Paris, UMR CNRS 8102, CNRS,LUTh, F-92190 Meudon, France., Univ Illinois, Dept Phys, Urbana, IL 61801 USA., Univ Illinois, Natl Ctr Supercomp Applicat, Urbana, IL 61801 USA., Heidelberg Inst Theoret Studies, D-69118 Heidelberg, Germany., Heidelberg Univ, Zentrum Astron, D-69120 Heidelberg, Germany., Univ Paris 06, UMR7095, Inst Astrophys Paris, F-75014 Paris, France., CNRS, UMR7095, Inst Astrophys Paris, F-75014 Paris, France., Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA., Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel., Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China., Univ Autonoma Madrid, Fac Ciencias, Dept Fis Teor, Modulo 15, E-28049 Madrid, Spain.

    المصدر: SCI

    Relation: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY.2013,435,(2),1618-1658.; 812298; http://hdl.handle.net/20.500.11897/391071; WOS:000325264600053

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    المصدر: Conselice, C J, Bluck, A F L, Mortlock, A, Palamara, D & Benson, A J 2014, ' Galaxy formation as a cosmological tool-I. The galaxy merger history as a measure of cosmological parameters ', Monthly Notices of the Royal Astronomical Society, vol. 444, no. 2, pp. 1125-1143 . https://doi.org/10.1093/mnras/stu1385

    وصف الملف: application/pdf

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    Academic Journal

    المساهمون: BAİBÜ, Fen Edebiyat Fakültesi, Matematik Bölümü, orcid:0000-0001-9673-8875, Özel, Cenap

    مصطلحات موضوعية: Dark Energy, Variable Lambda, Lambda-CDM Cosmology

    وصف الملف: application/pdf

    Relation: Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı; International Journal Of Theoretical Physics; https://doi.org/10.1007/s10773-008-9810-2; https://hdl.handle.net/20.500.12491/6537; 48; 373; 379