Type Ia supernovae have a consistent peak luminosity
Type Ia supernovae have a consistent peak luminosity
The discovery of dark energy through Type Ia supernovae observations has had a profound impact on our understanding of cosmology. It challenged the prevailing notion that the universe's expansion would eventually slow down due to gravitational forces. Instead, the presence of dark energy suggests a mysterious force driving the acceleration, reshaping our comprehension of the universe's fate and its ultimate destiny.
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The consistent peak luminosity of Type Ia supernovae was crucial for measuring cosmic distances and discovering the accelerating expansion of the universe, leading to the concept of dark energy.
Text adapted from Wikipedia, licensed under CC BY-SA 4.0.
Friedmann equations
Friedmann equations govern cosmic expansion in homogeneous and isotropic models
Dark energy
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Gunn–Peterson trough
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the CMB power spectrum tells us
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Chandrasekhar limit
Chandrasekhar limit is 1.4 solar masses
Gravitational lensing formalism
Light bends around massive objects due to spacetime curvature
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