The most mass of our Milky Way is contained in an inner region close to the core with radius Ro. Because the mass outside this inner region is almost constant, the density distribution can be written as following (assume a flat Milky Way with height z0): S Po, r< Ro 0, r> Ro p(r) = (a) Derive an expression for the mass M(r) enclosed within the radius r. (b) Derive the expected rotational velocity of the Milky Way v(r) at a radius r. (c) Astronomical observations indicate that the rotational velocity follows a different behaviour: Voba (r) = VGTP020 Ro 5/2 1+e-dr/R 4
The most mass of our Milky Way is contained in an inner region close to the core with radius Ro. Because the mass outside this inner region is almost constant, the density distribution can be written as following (assume a flat Milky Way with height z0): S Po, r< Ro 0, r> Ro p(r) = (a) Derive an expression for the mass M(r) enclosed within the radius r. (b) Derive the expected rotational velocity of the Milky Way v(r) at a radius r. (c) Astronomical observations indicate that the rotational velocity follows a different behaviour: Voba (r) = VGTP020 Ro 5/2 1+e-dr/R 4
College Physics
11th Edition
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Raymond A. Serway, Chris Vuille
Chapter1: Units, Trigonometry. And Vectors
Section: Chapter Questions
Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...
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Given
VIEWVisible mass distribution of the Milky way
VIEWExpected rotational velocity
VIEWExpected rotational velocity vs observed rotational velocity
VIEWRotational velocity due to the dark matter
VIEWRotational velocity due to the dark matter
VIEWRotational velocity due to dark matter.
VIEWDark matter mass distribution function
VIEWTheories in support of dark matter, Galaxy rotation curve and Gravitational lensing
VIEWLarge scale structure formation and the role of dark matter.
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