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Rozprawy doktorskie na temat „Cosmic microwave background radiation (CMB)”

Autor: Grafiati

Data publikacji: 3 czerwca 2025

Data aktualizacji: 31 lipca 2025

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1

Memari, Yasin. "Cosmological parameter estimation with QUaD CMB polarization and temperature experiment." Thesis, University of Edinburgh, 2009. http://hdl.handle.net/1842/4075.

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In this thesis we examine the theoretical origin and statistical features of the Cosmic Microwave Background radiation. We particularly focus on the CMB power spectra and cosmological parameter estimation from QUaD CMB experiment data in order to derive implications for the concordance cosmological model. In chapter 4 we present a detailed parameter estimation analysis of the combined polarization and temperature power spectra from the second and third season observations of the QUaD experiment. QUaD has for the first time detected multiple acoustic peaks in the polarization spectrum, allowing

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2

O'Sullivan, Creidhe Margaret Mary. "Observations of anisotropies in the CMBR at 15 GHz with the CAT." Thesis, University of Cambridge, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.389958.

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López-Caniego, Alcarria Marcos. "Detection of point sources in maps of the cosmic microwave background radiation by means of optimal filters." Doctoral thesis, Universidad de Cantabria, 2006. http://hdl.handle.net/10803/10647.

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Cuando observamos el cielo con los instrumentos más avanzados en la frecuencia de las microondas, los fotones que vemos fueron originados en regiones muy diferentes del universo. La mayoría proceden de nuestra propia galaxia (emisión difusa de sincrotrón, free-free y polvo), otros se originan en galaxias y cúmulos de galaxias muy lejanos, y, finalmente, una fracción tendrá su origen en la radiación del Big Bang, conocida como la Radiación del Fondo Cósmico de Microondas. Esta radiación está contaminada por las otras y su separación de ellas de una forma satisfactoria sigue siendo un problema a

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4

Kumar, Saurabh. "Radiating Macroscopic Dark Matter: Searching for Effects in Cosmic Microwave Background and Recombination History." Case Western Reserve University School of Graduate Studies / OhioLINK, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=case1606996786558263.

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5

Inman, Casey Ann. "A measurement of the cosmic microwave background radiation (CMBR) anisotropy at the half degree angular scale." Thesis, Massachusetts Institute of Technology, 1996. http://hdl.handle.net/1721.1/38384.

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6

Louis, Thibaut. "High resolution CMB physics." Thesis, University of Oxford, 2014. http://ora.ox.ac.uk/objects/uuid:b0d62439-37b8-4aa8-8d17-70141a70572a.

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This thesis presents the measurement of the cosmic microwave background (CMB) power spectrum for the Atacama Cosmology Telescope (ACT) experiment and its polarized upgrade, ACTPol. I present the tools that I have developed for constructing unbiased and nearly optimal statistical estimators. I discuss how to separate the cosmological and the astrophysical signal and how to characterize instrumental systematics. The goal of this work is to obtain accurate power spectra measurement that can be used for cosmological parameter estimation. I first present the analysis of the complete ACT data set. T

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7

Hancock, Stephen. "Detections of structure in the cosmic microwave background." Thesis, University of Cambridge, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.338307.

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8

Nazer, Mohammad Ahsan. "Cosmic microwave background anisotropies in an inhomogeneous universe." Thesis, University of Canterbury. Physics and Astronomy, 2015. http://hdl.handle.net/10092/10199.

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The timescape cosmology represents a potentially viable alternative to the standard homogeneous and isotropic Friedmann--Lemaître--Robertson--Walker (FLRW) cosmology, without the need for dark energy. This thesis first extends the previous work on the timescape cosmology to include a radiation component in the evolution equations for the timescape cosmology and tests of the timescape model are then performed against the Cosmic Microwave Background (CMB) temperature anisotropies from the Planck satellite. Although average cosmic evolution in the timescape scenario only differs substantial

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9

Dineen, Patrick. "Peculiar features in the cosmic microwave background radiation." Thesis, University of Nottingham, 2005. http://eprints.nottingham.ac.uk/10133/.

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In this thesis, I develop statistics capable of detecting peculiar features in current observations of the cosmic microwave background (CMB) radiation. Such tools scrutinise the very foundations of standard cosmological models. Evidence of peculiar features in the CMB may require a reassessment of these building blocks. More likely, any features may be artefacts of some non-cosmological signal. Nevertheless, whether the origin of these strange attributes is primordial or local, their discovery would be instructive. Existing statistical tools focus on the amplitude of the spherical harmonic coe

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10

Hervias, Caimapo Carlos. "Cosmology with CMB polarization : impact of foreground residuals." Thesis, University of Manchester, 2018. https://www.research.manchester.ac.uk/portal/en/theses/cosmology-with-cmb-polarization-impact-of-foreground-residuals(88d01ac3-65eb-43b5-a92d-fbbc28a59ff3).html.

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In this thesis, I present my work related to the characterization of diffuse Galactic foregrounds for observing the polarization of the Cosmic Microwave Background (CMB) radiation, and the impact of these foregrounds on the measurement of cosmological parameters. One of the most important future challenges for cosmology is the potential detection of polarization B-modes of the CMB. Inflation is a theory that explains the extremely early Universe, and solves several problems that were present in classical cosmology. It describes the anisotropies observed in the current Universe as primordial qu

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11

FORASTIERI, Francesco. "Probing the neutrino sector through Cosmic Microwave Background observations." Doctoral thesis, Università degli studi di Ferrara, 2018. http://hdl.handle.net/11392/2488088.

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Le interazioni tra neutrini oltre il modello standard della fisica delle particelle sono un campo aperto sia dal punto di vista teorico che sperimentale. In questa tesi presentiamo come le proprietà non standard dei neutrini possano essere vincolate usando le osservazioni cosmologiche e in particolare i dati della radiazione di fondo cosmica, come i dati di Planck. Considereremo la possibilità che i neutrini posseggano interazioni segrete scalari o pseudoscalari mediate da un bosone Nambu-Goldstone di una simmetria globale spontaneamente rotta U (1) ancora sconosciuta, come ad esempio i modell

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12

Osborne, Joshua C. P. "Eigenspectra for Correlating Cosmic Microwave Background Temperature Data." Case Western Reserve University School of Graduate Studies / OhioLINK, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=case1544180098307733.

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13

Su, Shi Chun. "Post-inflationary non-Gaussianities on the cosmic microwave background." Thesis, University of Cambridge, 2015. https://www.repository.cam.ac.uk/handle/1810/249054.

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The cosmic microwave background (CMB) provides unprecedented details about the history of our universe and helps to establish the standard model in modern cosmology. With the ongoing and future CMB observations, higher precision can be achieved and novel windows will be opened for studying different phenomena. Non-Gaussianity is one of the most exciting effects which fascinate many cosmologists. While numerous alternative inflationary models predict detectable primordial non-Gaussianities generated during inflation, the single-field slow-roll inflation of the standard model is known to produce

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14

Sollom, Ian Fraser. "Bayesian analysis of the CMB beyond the concordance model." Thesis, University of Cambridge, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.609814.

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15

Gruetjen, Helge Felix. "Optimal analysis of CMB anisotropies and polyspectra searches for primordial oscillatory features." Thesis, University of Cambridge, 2015. https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.709083.

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16

Regan, Donough Michael. "Measuring CMB non-Gaussianity as a probe of inflation and cosmic strings." Thesis, University of Cambridge, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.609806.

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17

O'Dwyer, Marcio. "Investigating Large Scale Anomalies of the Cosmic Microwave Background." Case Western Reserve University School of Graduate Studies / OhioLINK, 2020. http://rave.ohiolink.edu/etdc/view?acc_num=case1568822013962258.

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18

Dudley, Jonathan 1982. "Small-scale secondary anisotropies in the Cosmic Microwave Background." Thesis, McGill University, 2008. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=112618.

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One of the main harbingers of the modern age of precision cosmology, the Cosmic Microwave Background (CMB) has proven itself to be a veritable trove of cosmological information. With the aid of experiments such as the WMAP satellite, precision measurements of the CMB anisotropy spectra are now being made.<br>This work will first explore the physics of the Vishniac effect, a small-scale CMB temperature anisotropy created by the Compton scattering of CMB photons by free electrons caught in a line-of-sight bulk flow. The Vishniac effect arises due to a density enhancement in the electrons caused

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19

Legg, Stephen. "Multi-mode receiver systems for cosmic microwave background B-mode polarisation experiments." Thesis, University of Manchester, 2018. https://www.research.manchester.ac.uk/portal/en/theses/multimode-receiver-systems-for-cosmic-microwave-background-bmode-polarisation-experiments(11399beb-9f3d-455b-b236-7d612ab1a00b).html.

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A measurement of the primordial B-mode polarisation of the Cosmic Microwave Background would provide direct evidence of inflation in the early universe. The extremely weak nature of the B-mode signal necessitates an instrument with a high sensitivity and precise control over systematic effects. Multi-mode antenna feed horns offer higher sensitivity than their single-mode counterparts, however their behaviour is much more complex. The Short Wavelength Instrument for the Polarisation Explorer (SWIPE) onboard the Large Scale Polarisation Explorer (LSPE) is one instrument planning to implement mul

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20

Franzen, Thomas Matthew Owen. "Radio sources contaminating the CMB at 1 to 2 cm." Thesis, University of Cambridge, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.609365.

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21

Bevis, Neil Andrew. "Constraints on topological defects using the cosmic microwave background radiation." Thesis, University of Sussex, 2006. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.424400.

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22

Puchalla, Jason Lee. "Measuring cosmic microwave background radiation anisotropy on medium angular scales." Thesis, Massachusetts Institute of Technology, 1995. http://hdl.handle.net/1721.1/36965.

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23

Ma, Yin-Zhe. "Cosmology with CMB and large scale structure." Thesis, University of Cambridge, 2011. https://www.repository.cam.ac.uk/handle/1810/239394.

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Cosmology has become a precision science due to a wealth of new precise data from various astronomical observations. It is therefore important, from a methodological point of view, to develop new statistical and numerical tools to study the Cosmic Microwave Background (CMB) radiation and Large Scale Structure (LSS), in order to test different models of the Universe. This is the main aim of this thesis. The standard inflationary -dominated Cold Dark Matter ( CDM) model is based on the premise that the Universe is statistically isotropic and homogeneous. This premise needs to be rigorously teste

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24

Addison, Graeme Erik. "The clustering of dusty star-forming galaxies : connecting CMB cosmology and galaxy evolution." Thesis, University of Oxford, 2012. http://ora.ox.ac.uk/objects/uuid:3dff45be-9aa1-43c5-8c05-d1af84ff7010.

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In this thesis I construct various models to interpret measurements of the clustering of dusty star-forming galaxies through the angular power spectrum statistic. The goals of this work are, firstly, to facilitate the separation of the dusty galaxy contribution from the cosmic microwave background background (CMB) power spectrum, and, secondly, to improve our understanding of the physical properties of these galaxies. I present analysis of the first cross-correlation of millimeter and submillimeter sky maps, using data from the Atacama Cosmology Telescope (ACT) and the Balloon-borne Large-Aper

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25

Mcculloch, Mark Anthony. "Enhancing the noise performance of low noise amplifiers : with applications for future cosmic microwave background observatories." Thesis, University of Manchester, 2014. https://www.research.manchester.ac.uk/portal/en/theses/enhancing-the-noise-performance-of-low-noise-amplifiers--with-applications-for-future-cosmic-microwave-background-observatories(cd1da9b9-af7f-4bd2-a797-766c02855ab9).html.

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Low Noise Amplifiers (LNAs) are one of the most important components found in some of the radio receivers used in radio astronomy. A good LNA should simultaneously possess both a gain in excess of 25\,dB and as low a noise contribution as possible. This is because the gain is used to suppress the noise contribution of the subsequent components but the noise generated by the LNA adds directly to the noise of the overall receiver. The work presented in this thesis aimed to further enhance the noise performance through a variety of techniques with the aim of applying these techniques to the study

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26

Elsner, Franz. "Search for non-Gaussian Signatures in the Cosmic Microwave Background Radiation." Diss., lmu, 2010. http://nbn-resolving.de/urn:nbn:de:bvb:19-123086.

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27

Cartwright, John Kenneth Phinney E. Sterl Readhead Anthony C. S. "A limit on the polarization of the cosmic microwave background radiation /." Diss., Pasadena, Calif. : California Institute of Technology, 2003. http://resolver.caltech.edu/CaltechETD:etd-05292003-131234.

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28

Partridge, Bruce, Laura Bonavera, Marcos López-Caniego, et al. "Can CMB Surveys Help the AGN Community?" MDPI AG, 2017. http://hdl.handle.net/10150/625998.

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Contemporary projects to measure anisotropies in the cosmic microwave background (CMB) are now detecting hundreds to thousands of extragalactic radio sources, most of them blazars. As a member of a group of CMB scientists involved in the construction of catalogues of such sources and their analysis, I wish to point out the potential value of CMB surveys to studies of AGN jets and their polarization. Current CMB projects, for instance, reach mJy sensitivity, offer wide sky coverage, are blind and generally of uniform sensitivity across the sky (hence useful statistically), make essentially simu

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29

Aylor, K., Z. Hou, L. Knox, et al. "A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/626259.

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The Planck cosmic microwave background temperature data are best fit with a Lambda CDM model that mildly contradicts constraints from other cosmological probes. The South Pole Telescope (SPT) 2540 deg(2) SPT-SZ survey offers measurements on sub-degree angular scales (multipoles 650 <= l <= 2500) with sufficient precision to use as an independent check of the Planck data. Here we build on the recent joint analysis of the SPT-SZ and Planck data in Hou et al. by comparing Lambda CDM parameter estimates using the temperature power spectrum from both data sets in the SPT-SZ survey region. We also r

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30

Sayre, James. "Measuring Polarization of the Cosmic Microwave Background with the South Pole Telescope Polarization Experiment." Case Western Reserve University School of Graduate Studies / OhioLINK, 2014. http://rave.ohiolink.edu/etdc/view?acc_num=case1407351244.

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31

Pieroni, Mauro. "Classification of inflationary models and constraints on fundamental physics." Thesis, Sorbonne Paris Cité, 2016. http://www.theses.fr/2016USPCC258/document.

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Ce travail est concentré sur l'étude de la cosmologie primordiale et en particulier sur l'étude de l'inflation. Après une introduction sur la théorie standard du Big Bang, nous discutons de la physique du CMB et nous expliquons comment ses observations peuvent être utilisées pour définir des contraintes sur les modèles cosmologiques. Nous introduisons l'inflation et nous expliquons sa réalisation la plus simple. Nous présentons les observables et les contraintes expérimentales qui peuvent être utilisées pour mettre des contraintes sur les modèles d'inflation. La possibilité d'observer des onde

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32

Hoang, Thuong Duc. "Optimization of future projects for the measurement of Cosmic Microwave Background polarization." Thesis, Sorbonne Paris Cité, 2018. http://www.theses.fr/2018USPCC235.

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Au cours de ma thèse, mes recherches ont porté sur le développement des projets futurs de mesure de la polarisation du fond diffus cosmologique (CMB) visant à sonder les modes B primordiaux. Pour atteindre cet objectif, il faudra non seulement une sensibilité suffisante des matrices de détecteurs, mais également un contrôle sans précédent de toutes les erreurs systématiques inhérentes aux mesures de polarisation du CMB. Une source importante d’erreur systématique est la non-uniformité ou la non-concordance des filtres passe-bande des différents détecteurs. Cet effet induit des fuites de l’inte

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33

Bonaldi, Anna Valentina. "Component separation for all-sky CMB temperature maps." Doctoral thesis, Università degli studi di Padova, 2008. http://hdl.handle.net/11577/3426265.

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The work described in this Thesis is related to the PLANCK mission, scheduled for launch in 2008, which will observe the microwave sky with unprecedent resolution and sensitivity. The PLANCK collaboration involves hundreds of scientists and profits from the contributions of research groups in many countries. Among them, an Italian collaboration has a key role on component separation. This is a crucial step of the data reduction process, aimed at disentangling the Cosmic Microwave Background (CMB) and all the astrophysical components which are mixed in the nine observational channels of PLANCK

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34

Nagy, Johanna Marie Nagy. "Optical Development for the SPIDER Balloon-Borne CMB Polarimeter." Case Western Reserve University School of Graduate Studies / OhioLINK, 2017. http://rave.ohiolink.edu/etdc/view?acc_num=case1474029179516025.

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35

Rodríguez, Gonzálvez Carmen. "Analysis of cosmic microwave background observations with the Arcminute Microkelvin Imager." Thesis, University of Cambridge, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.609911.

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36

Carbone, Carmelita. "Non-linear structure formation and cosmic radiation backgrounds." Doctoral thesis, SISSA, 2007. http://hdl.handle.net/20.500.11767/4271.

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Modern cosmology begins with Einstein's 1917 paper where he applies his General Relativity (GR) Theory to Cosmology. After that day many discoveries have been performed and many successes in the theoretical knowledge have been achieved. Nowadays, the opinion of many physicists is that the Universe is well-described by what Fred Hoyle termed a Big Bang Model, according to which the Universe expanded from a denser hotter stage to its current state, where the present energy budget is dominated for ~ 76% the by dark energy and for ~ 20% by dark matter (neither of which have never been detected i

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37

Jones, William Claude Lange Andrew E. "A measurement of the temperature and polarization anisotropies of the cosmic microwave background radiation /." Diss., Pasadena, Calif. : California Institute of Technology, 2005. http://resolver.caltech.edu/CaltechETD:etd-05102005-102535.

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38

Ferté, Agnès. "Statistics of the CMB polarised anisotropies : unveiling the primordial universe." Thesis, Paris 11, 2014. http://www.theses.fr/2014PA112223/document.

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La compréhension des premiers instants de notre Univers complèterait notre description de son histoire et permettrait également une exploration de la physique fondamentale à des échelles d'énergie jusque là inatteignables. L'inflation cosmique est le scénario privilégié pour décrire ces premiers instants car il s'intègre très bien dans le modèle standard de la cosmologie. Selon ce scénario l'Univers aurait connu une courte période d'expansion accélérée peu après le Big Bang. Quelques indices favorisent ce modèle cependant toujours en attente d'une signature observationnelle décisive. Les modes

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39

Omori, Y., R. Chown, G. Simard, et al. "A 2500 deg2 CMB Lensing Map from Combined South Pole Telescope and Planck Data." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/626179.

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We present a cosmic microwave background (CMB) lensing map produced from a linear combination of South Pole Telescope (SPT) and Planck temperature data. The 150 GHz temperature data from the 2500 deg(2) SPT-SZ survey is combined with the Planck 143 GHz data in harmonic space to obtain a temperature map that has a broader l coverage and less noise than either individual map. Using a quadratic estimator technique on this combined temperature map, we produce a map of the gravitational lensing potential projected along the line of sight. We measure the auto-spectrum of the lensing potential C-L(ph

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40

Fung, Ho Ting. "A study of instrumental systematic effects due to quasi-optical components on CMB polarisation experiments." Thesis, University of Manchester, 2015. https://www.research.manchester.ac.uk/portal/en/theses/a-study-of-instrumental-systematic-effects-due-to-quasioptical-components-on-cmb-polarisation-experiments(0bef41e6-dd8c-4088-808d-826e8dfe939d).html.

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The new generation of astronomical instruments are not only in need of the highest sensitivity but require also well-controlled and known instrumental systematic effects. This is particularly relevant for projects dedicated to the study of the Cosmic Microwave background (CMB). Following the success of the Planck mission in providing the most detailed picture of the CMB temperature anisotropy to date, the next generation of CMB projects such as COrE (a potential future mission) and QUBIC (a ground based instrument)will be aiming to study the polarisation anisotropy of the CMB. However, the exp

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41

Rigaut, Olivier. "Nouveaux concepts pour les matrices de bolomètres destinées à l’exploration de l’Univers dans le domaine millimétrique." Thesis, Paris 11, 2014. http://www.theses.fr/2014PA112076/document.

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Depuis sa découverte en 1964, l’étude du Fond Diffus Cosmologique dans le domaine des longueurs d’ondes millimétriques est devenue un enjeu majeur de la recherche expérimentale dans le domaine de la cosmologie. En particulier, ses anisotropies en température, mesurées pour la première fois par le satellite COBE puis plus finement par l’expérience WMAP et le satellite PLANCK. L’existence prédite d’anisotropies de polarisation du Fond Diffus Cosmologique est fait actuellement parti du champ d’expérimentation privilégié de l’étude du CMB. En effet, la preuve d’existence des modes B de polarisatio

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42

SPINELLI, SEBASTIANO MAURO. "The use of optical coherence for instrumentation devoted to CMB experiments." Doctoral thesis, Università degli Studi di Milano-Bicocca, 2010. http://hdl.handle.net/10281/7884.

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The thesis discusses the application of the concept of optical coherence to novel instrumentation dedicated to the study of CMB. The complex degree of mutual coherence is used to describe the performances of QUBIC (Q and U Bolometric Interferometer for Cosmology, http://www.qubic.org). An adding, single baseline, interferometer prototype, working in the WR10 waveguide band, has been tested to investigate the basic properties of mm-wavelength bolometric interferometry in a mm-wave laboratory. Moreover the performances of the optical combiner of the final instrument are investigated. The cor

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43

Savage, Richard Stephen. "Searching for non-gaussianity in the cosmic microwave background radiation using the Very Small Array." Thesis, University of Cambridge, 2004. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.615771.

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44

Baskaran, Deepak. "Observational manifestations of gravitational waves in ground based interferometers and the Cosmic Microwave Background radiation." Thesis, Cardiff University, 2006. http://orca.cf.ac.uk/56098/.

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In this work we analyze two possible observational manifestations of gravitational waves. We consider the effects of gravitational waves on ground based laser interferometric detectors, and the imprints of relic gravitational waves on the Cosmic Microwave Background (CMB) radiation. In order to study the effect of a gravitational wave on a laser interferometer it is crucial to understand the movement of free test particles. The detailed knowledge of this motion is important conceptually and practically, because the mirrors of laser interferometric detectors of gravitational waves are essential

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45

Oppizzi, Filippo. "Non-Gaussianity in CMB analysis: bispectrum estimation and foreground subtraction." Doctoral thesis, Università degli studi di Padova, 2019. http://hdl.handle.net/11577/3425298.

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The focus of this work is the development of statistical and numerical methods forthe study of non-Gaussian and/or anisotropic features in cosmological surveys of themicrowave sky. We focus on two very different types of non-Gaussian (NG) signals. The former is primordial non-Gaussianity (PNG), generated in the very Early Universeduring the inflationary expansion stage. In this case the aim of our study will be that ofexploiting the NG component in order to extract useful cosmological information. The latter is non-Gaussianity generated by astrophysical foreground contamination. In thiscase,

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Vanneste, Sylvain. "Constraints on primordial gravitational waves from the large scales CMB data." Thesis, Université Paris-Saclay (ComUE), 2019. http://www.theses.fr/2019SACLS314/document.

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Cette thèse s’articule autour du développement d'outils d’analyse des modes B du fond diffus cosmologique (CMB) dans le but d'estimer l’amplitude des ondes gravitationnelles primordiales produites durant la période inflationnaire.Nous nous intéressons plus précisément aux grandes échelles angulaires, pour lesquelles le signal attendu des modes B primordiaux est dominant. Ces échelles étant particulièrement contaminées par des émissions polarisées galactiques, nous avons étudié et développé des méthodes permettant de réduire ces contaminations et de caractériser les résidus. Ces outils peuvent

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Obranovich, Michael A. "The effects of non-zero neutrino masses on the CMB determination of the cosmological parameters." The Ohio State University, 2012. http://rave.ohiolink.edu/etdc/view?acc_num=osu1337799009.

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Dani, Gerd. "Esperimenti per la misura della radiazione cosmica di fondo a microonde." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2016. http://amslaurea.unibo.it/12326/.

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In cosmologia, la radiazione cosmica di fondo a microonde abbreviata spesso in CMB, dall'inglese Cosmic Microwave Background Radiation, è la radiazione elettromagnetica residua prodotta dal Big Bang che permea l'Universo. A partire dagli anni ’60 fino ad oggi, centinaia sono stati gli esperimenti (da Terra e da Spazio) che hanno permesso di ottenere sempre più informazioni sulla radiazione cosmica via via con sempre maggiore sensibilità e accuratezza. Grazie ai risultati ottenuti, è possibile ad oggi confermare la bontà della teoria inflazionaria e comprenderne meglio l’evoluzione temporale d

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Staniszewski, Zachary K. "First Galaxy Clusters Discovered Via the Sunyaev Zel-D'ovich Effect /." Cleveland, Ohio : Case Western Reserve University, 2010. http://rave.ohiolink.edu/etdc/view?acc_num=case1271698482.

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Thesis (Doctor of Philosophy)--Case Western Reserve University, 2010<br>Department of Physics Title from PDF (viewed on 2010-05-25) Includes abstract Includes bibliographical references and appendices Available online via the OhioLINK ETD Center

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Reichardt, Christian L. Lange Andrew E. Lange Andrew E. "A high resolution measurement of temperature anisotropies in the cosmic microwave background radiation with the complete ACBAR data set /." Diss., Pasadena, Calif. : California Institute of Technology, 2008. http://resolver.caltech.edu/CaltechETD:etd-12202007-130152.

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