CMB anisotropy due to filamentary gas: Power spectrum and cosmological parameter bias

Keyphrases

• Power Spectrum 100%
• Statistical Uncertainty 100%
• Cosmological Parameters 100%
• Parameter Bias 100%
• Spectrum Parameter 100%
• CMB Experiments 100%
• CMB Anisotropy 100%
• Power-to-gas 100%
• Survey Data 50%
• Scalar 50%
• Planck 50%
• Hot Gas 50%
• Anisotropy 50%
• Morphological Properties 50%
• Power Level 50%
• N-body Simulations 50%
• Filamentary Structure 50%
• Gas Properties 50%
• Primordial Power Spectrum 50%
• Intrinsic Interest 50%
• Angular Scales 50%
• Irregular Morphology 50%
• Equation of State Parameter 50%
• SZ Effect 50%
• Dark Energy Equation of State 50%
• Cosmological Parameter Estimation 50%

Physics

• Anisotropy 100%
• Power Spectra 100%
• Cosmological Parameters 100%
• Equations of State 33%
• High Temperature Gas 33%
• Multipole 33%
• N-Body Simulations 33%
• Parameter Estimation 33%