Obstacle
发表于 2025-3-28 17:44:13
Die Entwicklung in der 1. Republikng measurements of the geometry, constitution, and early history of the universe. Future CMB anisotropy observations allow a stringent test of cosmological models and a precision determination of cosmological parameters of its standard model.
帐单
发表于 2025-3-28 22:00:07
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平躺
发表于 2025-3-29 01:08:42
Inès Ajmi,Hayfa Zgaya,Slim HammadiE-DMR maps of the cosmic microwave background anisotropy measure the primordial density distribution on super-horizon scales and offer a unique probe of the “initial conditions” for structure formation. I will present several statistical tests of the large-scale CMB anisotropy, with an emphasis on what what we can learn, what we can’t, and why.
Excitotoxin
发表于 2025-3-29 04:50:17
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壁画
发表于 2025-3-29 08:07:44
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Circumscribe
发表于 2025-3-29 12:28:09
Cosmic Microwave Background Anisotropy Scienceng measurements of the geometry, constitution, and early history of the universe. Future CMB anisotropy observations allow a stringent test of cosmological models and a precision determination of cosmological parameters of its standard model.
我要威胁
发表于 2025-3-29 16:51:13
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大喘气
发表于 2025-3-29 22:46:35
Large-Scale Anisotropy of the Cosmic Microwave BackgroundE-DMR maps of the cosmic microwave background anisotropy measure the primordial density distribution on super-horizon scales and offer a unique probe of the “initial conditions” for structure formation. I will present several statistical tests of the large-scale CMB anisotropy, with an emphasis on what what we can learn, what we can’t, and why.
人造
发表于 2025-3-30 03:30:57
https://doi.org/10.1007/978-3-211-74420-8tic theory may arise at one loop order. Using the wordline representation of the one loop effective action, I follow D’Hoker and Gagné to replace the Wilson line by an integral over worldline fermions. A bilinear of these worldline fermions naturally defines a nonabelian charge, whose equation of motion is Wong’s equation.
Sarcoma
发表于 2025-3-30 05:47:55
Gegenüberstellung mit der Vorausgabefor temperatures near and above the critical temperature. Electroweak baryogenesis during this transition seems not possible within the standard model. The observed baryon asymmetry in the universe therefore implies the necessity of an extension of the standard model.