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Intro
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AIM OF MY LECTURES: UNDERSTAND THIS PLOT
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OUTLINE LECTURE 1
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THRESHOLD FOR PAIR PRODUCTION
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CROSS SECTION FOR PAIR PRODUCTION
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BACKGROUND RADIATION FIELDS
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EBL MEASUREMENTS
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INGREDIENTS TO THE EBL: STARS
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ADDITIONAL CONTRIBUTIONS?
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EBL MODELS
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OPTICAL DEPTH
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CONSTRAINING THE EBL WITH GAMMA-RAY OBSERVATIONS
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MODEL THE EBL INGREDIENTS DIRECTLY
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CONCLUSIONS y-RAY ABSORPTION
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PARITY TRANSFORMATION
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CHARGE-PARITY
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AXION SOLVES THE STRONG CP PROBLEM
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AXIONLIKE PARTICLES (ALPs)
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EVOLUTION OF AXION/ALP FIELD IN AN EXPANDING UNIVERSE
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THE AXION / ALP PARAMETER SPACE
Description:
Save Big on Coursera Plus. 7,000+ courses at $160 off. Limited Time Only! Grab it Explore fundamental physics concepts in this comprehensive lecture from the Latin-American School on CTA Science. Delve into topics such as pair production thresholds, cross-sections, background radiation fields, and extragalactic background light (EBL) measurements. Examine the role of stars in EBL composition, various EBL models, and optical depth. Learn how gamma-ray observations can constrain EBL and discover direct modeling techniques for EBL ingredients. Investigate parity transformation, charge-parity, and the strong CP problem. Gain insights into axions and axion-like particles (ALPs), their evolution in an expanding universe, and the axion/ALP parameter space. Enhance your understanding of fundamental physics principles and their applications in astrophysics and cosmology.

Fundamental Physics: Gamma-Ray Absorption and Axion-Like Particles - Class 1

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