Transcription of A Concise Introduction to Astrophysics
{{id}} {{{paragraph}}}
A Concise Introduction to Astrophysics Lecture Notes for FY2450 M. Kachelrie M. Kachelrie Institutt for fysikkNTNU, TrondheimNorwayemail: M. Kachelrie 2008, minor corrections Stellar astrophysics101 Continuous radiation from Brightness of stars .. Color of stars .. Black-body radiation .. Kirchhoff-Planck distribution .. Wien s displacement law .. Stefan-Boltzmann law .. Spectral energy density of a photon gas .. Stellar distances .. Stellar luminosity and absolute magnitude scale .. 182 Spectral lines and their Bohr-Sommerfeld model for hydrogen-like atoms.
– The need for a new form of “dark matter” to describe correctly the formation and dynamics of galaxies requires a yet unknown extension of the current standard model of elementary particle physics. The same holds true for a new form of ”dark energy” required for the explanation of the accelerated expansion of the universe.
Domain:
Source:
Link to this page:
Please notify us if you found a problem with this document:
{{id}} {{{paragraph}}}