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A great place to be

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Greetings and salutations

They said senior year would be a breeze. To avoid such a horrifying prospect, I decided to indulge in AP-C Physics, which, as they say, is one of the most challenging classes the school has to offer. But, as the Chinese proverb goes, "The gem cannot be polished without friction, nor man perfected without trials". I am not taking AP-C Physics simply because I enjoy torturing myself with hard problems. In actuality, I hope to be able to tackle hard problems step-by-step. There is always a logic

jelliott

jelliott

Guitar Physics (String Bending)

I made a post a while back about the physics behind pinch harmonics - but, since there is a multitude of other guitar techniques, there's a lot more physics to be explored with this instrument. Think about your all-time favorite guitar solo, and I'll guarantee you that there is bending somewhere in it. It's the technique that must be mastered to make a decent solo, and it's in all of the best ones: it's ever-present in legendary solos such as Pink Floyd's "Comfortably Numb", Lynyrd Skynyrd's

jelliott

jelliott

Guitar Physics (Whammy Bars)

My last one, I promise. When I stumbled upon Mr. Grimes' paper regarding all of these guitar applications to physics, I had already known that things like harmonics had to do with basic string/wave physics - but all of these other applications have really interested me, as someone who loves the instrument. If you're interested at all, visit the source material; he obviously worked very hard on it, and his hard work shines through. http://www.plosone.org/article/info%3Adoi%2F10.1371%2Fjourn

jelliott

jelliott

Orbital Decay and You

(You, of course, indicating its impact on the Earth and not necessarily you on a personal level.) By essentially sapping energy from an orbital system, gravitational radiation makes orbits more circular and continuously decreases their radii. Overall angular momentum decreases, as this too is essentially stolen by radiation. The decrease in the radius of orbit is given by the following equation: Substitution of the Earth's and Sun's masses for m1 and m2 tells us that the rate of our orbit

jelliott

jelliott

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