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1
Introduction
2
Stars as a laboratory
3
The method
4
Energy conservation equations
5
Theoretical errors
6
Globular clusters
7
HR diagrams
8
What we need
9
Theory
10
Model A
11
Results
12
Historical evolution
13
The number of stars
14
The air parameter
15
Error analysis
16
Combined analysis
17
Massive stars
18
Supergiants
19
Supernovae
20
Collapse
21
Result
22
Conversion
23
Satellite
24
Vera Rubin
Description:
Explore the future of axion astrophysics in this comprehensive 1-hour 15-minute lecture by Oscar Straniero at the Galileo Galilei Institute. Delve into the potential of using stars as laboratories to study axions, examining energy conservation equations and theoretical errors. Investigate globular clusters and HR diagrams, discussing the necessary theoretical models and parameters for accurate analysis. Learn about the historical evolution of axion research, including the importance of massive stars, supergiants, and supernovae in this field. Discover the latest results from combined analyses and error assessments, and gain insights into the role of satellites like Vera Rubin in advancing our understanding of axions in astrophysics.

The Future of Axion Astrophysics - What Can We Learn About Axions from Future Astrophysical Probes

Galileo Galilei Institute
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