Recent content by fhqwgads2005

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    Energies of a particle in a box vs. free particle?

    Interesting... maybe one day I'll learn relativistic QM...
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    Energies of a particle in a box vs. free particle?

    Hmm, so is there a relatively simple way to think about the particle in a box including relativity?
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    Energies of a particle in a box vs. free particle?

    I think I'm trying to reconcile quantum mechanics and special relativity . . . or whatever I'm doing I'm pretty confused. Ok, so the allowed energy states for a particle in a box are E_n = \frac{\hbar^2 \pi^2}{2 m L^2} n^2 . This seems to mean, as you increase the length L, the particle's...
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    General equation for the speed of sound?

    I've seen stated in many a physics book that the general case for the speed of sound (for general equations of state p(ρ) ) is given by c^2 = \frac{\partial p}{\partial \rho} where p is pressure and ρ is density. but I can't for the life of me figure out how on Earth to derive that...
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    What is nuclear symmetry energy?

    So, is it useful to think of it as the energy required to increase the asymmetry between N and Z in the nucleus, say, by electron capture?
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    Neutron Star Below the Chandrasehkar Limit - Properties & Atomic Matter?

    How does this relate to the final mass of the neutron star? Does the star accrete another .7 solar mass of matter after the supernova explosion? Or during it at some point? Also, can anyone point me towards up to date information regarding the current status of neutron star EOS's, like, which...
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    Discovering the Universe's Flatness: Insights from an Amateur Astronomer

    I meant theoretically... you can prove through the math of GR that the universe flattened by a factor of something like 10^60 after inflation. Observationally of course, we can only tell it's flat to something like 0.5% uncertainty.
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    Discovering the Universe's Flatness: Insights from an Amateur Astronomer

    Ahh, I think you mean the raw microwave images. The line you see in the middle is just due to the microwaves produced by our own galaxy. These aren't part of the CMB, even though they give off the same wavelengths. That big line in the middle is usually removed using complex statistical...
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    Physics Renewable energy jobs with a BS in physics

    Out of curiosity, what kind of work/responsibilities did you have? Did you feel like your physics background was a benefit? Looking around at listings from various renewable energy companies, every job I've seen requires either an engineering background or some technical background like...
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    Physics Renewable energy jobs with a BS in physics

    Im graduating with a BS in physics, where I mostly focused on astrophysics. I'm looking to do something different after I graduate, not planning on grad school, at least for the time being. I'm interested in getting a job somehow related to renewable energy technology, and it would also be a...
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    Physics Leaving Physics MSc: After Physics BSc, What Next?

    Just out of curiosity, what type of undergraduate coursework is usually required to get into a MS engineering program? I'm graduating with a BS in physics, I can't find any info on what schools expect candidates to have taken beforehand...
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    Discovering the Universe's Flatness: Insights from an Amateur Astronomer

    I'm not sure what you mean by the condensed line... The CMB is very uniform throughout the universe, except for very small local fluctuations called anisotropies. These are used to determine the energy densities of the universe, and from that, the geometry. Expansion has no direction, the...
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    Discovering the Universe's Flatness: Insights from an Amateur Astronomer

    The concept of "flat" geometry is a little difficult to picture in 3 dimensions, in fact, it really is impossible. The best one can do is think about the implications of things being flat or curved. For now, let's just think of the universe as having 2 spatial dimensions. So let's just say...
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    Neutron Star Below the Chandrasehkar Limit - Properties & Atomic Matter?

    Let's say the Fe core reaches the Chandrasekhar limit. It begins to collapse, and at some point, the very center of the core will reach the neutron degeneracy limit. However, some parts of the core must continue to collapse inwards, until they too reach the neutron degeneracy pressure limit...
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