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Probing the High-Redshift Universe Using Fluctuations in the Cosmic Microwave and Infrared Backgrounds.

机译：使用宇宙微波和红外背景下的涨落来探测高红移宇宙。

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Background (CIB) continues to be one of the best probes of physics at the early stages of the universe. If the CMB were a purely Gaussian field, all statistical information would be contained in the power spectrum or two-point correlation function. However, non-Gaussianities ensure that new physics may be extracted from higher n-point correlation functions including the bispectrum and trispectrum of the CMB. In this thesis discuss new estimators we have formulated to probe primordial non-Gaussianity in the bispectrum and trispectrum of CMB data and the constraints we have made using WMAP data while discussing implications for inflationary models. I discuss how these same methods may be used to probe CMB Lensing. Finally, I discuss how upcoming measurements of near and far-infrared CIB fluctuations may be used to constrain the redshift of reionization and clustering of various populations of galaxies. Some preliminary results involving CANDELS, Spitzer SDWFS, CIBER and Herschel datasets is presented.

机译：背景技术（CIB）仍然是宇宙早期对物理的最好探索之一。如果CMB是纯高斯场，则所有统计信息都将包含在功率谱或两点相关函数中。然而，非高斯性确保可以从更高的n点相关函数（包括CMB的双谱和三谱）中提取新的物理学。在本文中，我们讨论了新的估计量，我们在探讨CMB数据的双谱和三谱中的原始非高斯性以及我们在讨论通货膨胀模型的含义时使用WMAP数据所做的约束时探讨了这些估计。我将讨论如何使用这些相同的方法来探测CMB Lensing。最后，我讨论了即将到来的近红外和远红外CIB波动的测量结果可如何用于约束不同星系群体的电离和聚类的红移。提出了一些涉及CANDELS，Spitzer SDWFS，CIBER和Herschel数据集的初步结果。

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作者
Smidt, Joseph Michael.;
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University of California, Irvine.;

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授予单位 University of California, Irvine.;
学科 Physics Astrophysics.;Physics General.
学位 Ph.D.
年度 2012
页码 217 p.
总页数 217
原文格式 PDF
正文语种 eng
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1. ON THE ABSENCE OF ANTIMATTER FROM THE UNIVERSE, DARK MATTER, THE FINE STRUCTURE PARAMETER, THE FLUCTUATIONS OF THE COSMIC MICROWAVE BACKGROUND RADIATION AND THE TEMPERATURE DIFFERENCE BETWEEN THE NORTHERN AND SOUTHERN HEMISPHERE OF THE UNIVERSE [J] . Emmanuil Manousos Physics International . 2014,第1期

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2. ON THE ABSENCE OF ANTIMATTER FROM THE UNIVERSE, DARK MATTER, THE FINE STRUCTURE PARAMETER, THE FLUCTUATIONS OF THE COSMIC MICROWAVE BACKGROUND RADIATION AND THE TEMPERATURE DIFFERENCE BETWEEN THE NORTHERN AND SOUTHERN HEMISPHERE OF THE UNIVERSE | Science Publications [J] . Emmanuil Manousos Physics International . 2014,第1期

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3. ON THE ABSENCE OF ANTIMATTER FROM THE UNIVERSE, DARK MATTER, THE FINE STRUCTURE PARAMETER, THE FLUCTUATIONS OF THE COSMIC MICROWAVE BACKGROUND RADIATION AND THE TEMPERATURE DIFFERENCE BETWEEN THE NORTHERN AND SOUTHERN HEMISPHERE OF THE UNIVERSE [J] . Emmanuil Manousos Physics International . 2013,第2期

机译：关于宇宙的反作用物质，暗物质，精细结构参数，宇宙微波背景辐射的波动以及宇宙南北半球之间的温度差异
4. Interaction-Powered Supernovae as Probes of the High-Redshift Universe [C] . Takashi Moriya, Naoki Yoshida, Nozomu Tominaga, International Conference "The Stars and Galaxies: Challenges for the Next Decade" . 2010

机译：相互作用的超新星作为高射频宇宙的探头
5. Future Probes of Cosmology and the High-Redshift Universe. [D] . Visbal, Elijah Francis. 2013

机译：宇宙学和高红移宇宙的未来探索。
6. ETHOS – an effective theory of structure formation: predictions for the high-redshift Universe – abundance of galaxies and reionization [O] . Mark R. Lovell, Jesús Zavala, Mark Vogelsberger, -1

机译：ETHOS –一种有效的结构形成理论：对高红移宇宙的预测–星系的丰富和电离
7. Power Asymmetry in Cosmic Microwave Background Fluctuations from Full Sky to Sub-Degree Scales: Is the Universe Isotropic? [O] . Hansen F. K., Banday A. J., Górski K. M., 2009

机译：从满天到近度尺度的宇宙微波背景波动中的功率不对称：宇宙各向同性吗？
8. Contribution of z < 6 Sources to the Spatial Coherence in the Unresolved Cosmic Near-Infrared and X-Ray Backgrounds. [R] . Helgason, K., Cappelluti, N., Hasinger, G., 2014

机译：z <6源对未解析的宇宙近红外和X射线背景中空间相干性的贡献。

Probing the High-Redshift Universe Using Fluctuations in the Cosmic Microwave and Infrared Backgrounds.

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