Recent content by Fabio010

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    Check if the complex function is differentiable

    The question is to check where the following complex function is differentiable. w=z \left| z\right| w=\sqrt{x^2+y^2} (x+i y) u = x\sqrt{x^2+y^2} v = y\sqrt{x^2+y^2} Using the Cauchy Riemann equations \frac{\partial }{\partial x}u=\frac{\partial }{\partial y}v...
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    How to check if function is differentiable at a point

    The question is to check where the following complex function is differentiable. w=z \left| z\right| w=\sqrt{x^2+y^2} (x+i y) u = x\sqrt{x^2+y^2} v = y\sqrt{x^2+y^2} Using the Cauchy Riemann equations \frac{\partial }{\partial x}u=\frac{\partial }{\partial y}v...
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    Solve Hubble's Law: Proxima Centauri & Sun in Milky Way

    Yes, your are right. "Away from the central bulge or outer rim, the typical stellar orbital speed is between 210 and 240 km/s" Instead of 828km/h it is 828000km/h Thanks for the help!
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    Solve Hubble's Law: Proxima Centauri & Sun in Milky Way

    Homework Statement Determine for the nearest star what should be it's recessional velocity if the space between the two stars is expanding according to the Hubble's law. Compare this value with the speed of the sun when it moves with Milk Way. Homework Equations H_{0} = \frac {v}{D}...
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    Dark matter density in fucntion of radius

    Thanks for the help mfb!
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    Cosmic microwave background radiation

    Understood! Thanks a lot for the help!
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    Cosmic microwave background radiation

    So, the difference is the switching from wavelength to frequency dependence. The results are "mathematically" equal?
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    Dark matter density in fucntion of radius

    So with my result, i can conclude that the dark matter density decreases with the distance from the center of the galaxy. But is not the dark matter suppose to increase with the distance? To maintain the galaxy rotation velocity constant?
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    Dark matter density in fucntion of radius

    like this: \vec{} F=\frac{GMm}{R^{2}} a=\frac{v^{2}}{R} The Attempt at a Solution \frac{F}{m}=\frac{GM}{R^{2}} 4\pi \frac{F}{m}=\frac{4\pi GM}{R^{2}} \frac{v^{2}}{R}=\frac{GM}{R^{2}} dM=4\pi\rho (R)R^{2}dR dM=\frac{v^{2}}{G}dR 4\pi\rho (R)R^{2}dR=\frac{v^{2}}{G}dR...
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    Cosmic microwave background radiation

    Homework Statement The cosmic microwave background radiation has a blackbody type spectrum. Determine its max frequency and the correspondent wavelenght. Verify if found frequency is a microwave frequency and compare with the following curve: Homework Equations Using the...
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    Dark matter density in fucntion of radius

    Homework Statement Evidence for dark matter comes from “flat” rotation curves of galaxies. Assume that the observed matter moves in circular orbits about the center of the galaxy and that the velocity of the matter as a function of the radius v(r) is a constant. Also assume...
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    How do frequency and pressure affect sound in Kundt's Tube?

    Homework Statement Kundt's Tube.First of all, i used a aluminum rod. Then i rubbed it to cause vibration . Homework Equations a)How can i change the frequency of the sound produced in tube. b)What is the difference of rubbing the metal with more pressure?The Attempt at a Solution a)...
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    Electric field inside a polarized sphere

    So you are telling me that \vec{E}(A) = \frac{∫-∇.\vec{P}dv}{εo}
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    Electric field inside a polarized sphere

    Homework Statement A sphere of radius R carries a polarization \vec{P}= k\vec{r}, where k is a constant and \vec{r} is the vector from the center. Find the field inside and outside the sphere. In solution, the field outside sphere is 0. I interpreted that as the field...
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