Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations.
Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations.
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DOI：
10.1103/physrevlett.86.3475
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发表时间：
2000-07
影响因子：
8.6
通讯作者：
A. Jaffe;P. Ade;A. Balbi;J. Bock;J. Bond;J. Borrill;A. Boscaleri;K. Coble;B. Crill;P. Bernardis;P. Farese;P. Ferreira;K. Ganga;M. Giacometti;S. Hanany;E. Hivon;V. Hristov;A. Iacoangeli;A. Lange;Adrian T. Lee;L. Martinis;S. Masi;P. Mauskopf;A. Melchiorri;T. Montroy;C. Netterfield;Sang-Yun Oh;E. Pascale;F. Piacentini;D. Pogosyan;S. Prunet;B. Rabii;S. Rao;P. Richards;G. Romeo;J. Ruhl;F. Scaramuzzi;D. Sforna;G. Smoot;R. Stompor;C. Winant;Jiun-Huei Proty Wu
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文献类型：
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作者：
A. Jaffe;P. Ade;A. Balbi;J. Bock;J. Bond;J. Borrill;A. Boscaleri;K. Coble;B. Crill;P. Bernardis;P. Farese;P. Ferreira;K. Ganga;M. Giacometti;S. Hanany;E. Hivon;V. Hristov;A. Iacoangeli;A. Lange;Adrian T. Lee;L. Martinis;S. Masi;P. Mauskopf;A. Melchiorri;T. Montroy;C. Netterfield;Sang-Yun Oh;E. Pascale;F. Piacentini;D. Pogosyan;S. Prunet;B. Rabii;S. Rao;P. Richards;G. Romeo;J. Ruhl;F. Scaramuzzi;D. Sforna;G. Smoot;R. Stompor;C. Winant;Jiun-Huei Proty Wu
最近的结果从BOOMERANG-98和MAXIMA-1，与COBE DMR一起，提供了一致的和高信噪比测量的宇宙微波背景功率谱在球谐多极带超过2 <l不太相似800。对组合数据的分析得出总密度的置信限为68%（95%），Omega（tot）约为1.11 +/-0.07（+0.13）（-0.12），重子密度，Ω（B）h（2）约为0.032（+0.005）（-0.004）（+0.009）（-0.008），以及标量频谱倾斜，n（s）约为1.01（+0.09）（-0.07）（+0.17）（-0.14）。这些数据与结构形成的暴胀初始条件是一致的。与其他宇宙学观测结果一起，它们意味着宇宙中存在非重子暗物质和暗能量。
Recent results from BOOMERANG-98 and MAXIMA-1, taken together with COBE DMR, provide consistent and high signal-to-noise measurements of the cosmic microwave background power spectrum at spherical harmonic multipole bands over 2<l less similar to 800. Analysis of the combined data yields 68% (95%) confidence limits on the total density, Omega(tot) approximately 1.11+/-0.07 (+0.13)(-0.12), the baryon density, Omega(b)h(2) approximately 0.032(+0.005)(-0.004) (+0.009)(-0.008), and the scalar spectral tilt, n(s) approximately 1.01(+0.09)(-0.07) (+0.17)(-0.14). These data are consistent with inflationary initial conditions for structure formation. Taken together with other cosmological observations, they imply the existence of both nonbaryonic dark matter and dark energy in the Universe.