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Guided learning journeys that build knowledge step by step.
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This path guides graduate students in cosmology through the conceptual and technical connections between cosmology and string theory. It covers essential string theory concepts, extra dimensions, moduli stabilization, and string-inspired early universe scenarios, providing a clear learning sequence from prerequisites to advanced topics.
This advanced graduate-level path explores the multiverse concept in cosmology, from its roots in inflationary theory and quantum field theory to specific proposals like eternal inflation and the string landscape. It critically examines observational signatures, scientific testability, and philosophical implications, equipping learners to evaluate the multiverse's scientific status.
This advanced graduate path equips learners to use gravitational waves (GWs) as cosmological tools, covering necessary physics, data analysis, and applications to measure cosmic expansion and test gravity. It progresses from foundational GR and GW theory through detection and analysis to specific cosmological applications, culminating in the stochastic GW background.
A graduate-level learning path that equips cosmology students with the machine learning skills needed to tackle modern cosmological problems. It covers essential ML concepts, cosmological data analysis, and specific applications including classification, parameter estimation, generative models, and anomaly detection. The path emphasizes practical implementation with Python and deep learning frameworks.
This advanced graduate-level path develops the theoretical framework for understanding the large-scale structure of the universe, from linear perturbation theory to effective field theory approaches. It covers the statistical tools, bias models, nonlinear evolution, redshift-space distortions, and BAO modeling essential for modern cosmological analysis. The path emphasizes the conceptual connections between cosmology, field theory, and statistical physics, preparing learners for research in theoretical cosmology.
This advanced graduate-level path covers the end-to-end design of instruments for cosmological observations, including CMB detectors, radio telescopes, optical surveys, and space missions. Learners will gain expertise in cryogenics, readout systems, calibration, and data analysis methods, with a strong foundation in detector physics and electronics.
This learning path equips graduate students in cosmology with the skills to use simulation-based inference (likelihood-free inference) for cosmological parameter estimation. It covers forward modeling, emulators, approximate Bayesian computation, and neural network approaches, culminating in applied projects that constrain cosmological parameters from simulated data.
A graduate-level learning path covering the statistical and computational techniques required to extract cosmological parameters from combined datasets. It progresses from probability theory and Bayesian inference through likelihood construction, sampling methods, and advanced topics such as parameter degeneracies, model comparison, and tension quantification.
This learning path guides graduate students in cosmology through the essential concepts and practical skills required to perform weak lensing measurements. It covers gravitational lensing theory, shape measurement, PSF correction, shear calibration, two-point statistics, and systematics tests, culminating in the application of shear ratios.
This learning path equips graduate students in cosmology with the skills to analyze large-scale galaxy survey data, from survey design and target selection through redshift measurements to clustering statistics, BAO, and RSD measurements. It emphasizes practical applications using modern surveys like eBOSS and DESI, integrating statistical methods and software development.