Recent content by Frostman
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Charge invariance with Heaviside's function
In the first step you indicated all the primate terms, except ##\eta_\beta## because I must be able to reduce to the definition of charge as a three-dimensional integral of ##J'^0##. I then observe that in reality the other primate quantities are Lorentz invariants. When I exchange the...- Frostman
- Post #17
- Forum: Advanced Physics Homework Help
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Charge invariance with Heaviside's function
$$d^4x'=\bigg|\frac{\partial x'}{\partial x}\bigg|d^4x$$ Where ##\bigg|\frac{\partial x'}{\partial x}\bigg|## is the determinant of jacobian of Lorentz-transformation, for the Lorentz proper transformation ##det\Lambda^\mu{}_\nu=1##. The demonstration I am following is that of Weinberg chapter...- Frostman
- Post #15
- Forum: Advanced Physics Homework Help
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Charge invariance with Heaviside's function
Perfect, one last step and I believe I am there. Given this definition of charge Q we have that $$Q'=\int d^4x J^\alpha(x)\partial_\alpha \theta(\eta_\beta'x^\beta)$$ For ##J_\alpha\partial_\alpha## I understood because the product of a covariant and contravariant four-vector is a relativistic...- Frostman
- Post #13
- Forum: Advanced Physics Homework Help
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Charge invariance with Heaviside's function
Yes, I corrected, I forgot a zero. Excuse me, but this is my first time working with the Heaviside and Dirac delta function together. $$\partial_0\theta(x^0)=\delta(x^0)$$ Is it correct? $$\int d^3x \int dx^0J^0(x^0, \vec x) \delta(x^0)$$ Or can I suppose that ##\delta(x^0) =...- Frostman
- Post #11
- Forum: Advanced Physics Homework Help
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Charge invariance with Heaviside's function
Can I proceed like this to reduce it to the 3D relationship? $$Q=\int dx^0d^3x J^0(x)\partial_0\theta(x^0)=\int d^3x J^0(x)dx^0\partial_0\theta(x^0)=\int d^3x J^0(x)$$- Frostman
- Post #9
- Forum: Advanced Physics Homework Help
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Charge invariance with Heaviside's function
The only derivative ##\partial_\alpha## that can act is only this one ##\partial_0##. So it remains $$Q=\int d^4x J^0(x)\partial_0\theta(x^0)$$- Frostman
- Post #7
- Forum: Advanced Physics Homework Help
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Charge invariance with Heaviside's function
The only term that remains is ##x^0## because ##\eta_\beta## is defined as ##\eta_\beta=(1,0,0,0)## So ##\theta(\eta_\beta x^\beta)=\theta(\eta_0x^0)=\theta(x^0)##- Frostman
- Post #5
- Forum: Advanced Physics Homework Help
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Charge invariance with Heaviside's function
I hope I understand the definition of the Heaviside function well For ##\beta=0##, ##\theta(\eta_\beta x^\beta)=1## For ##\beta\neq0##, ##\theta(\eta_\beta x^\beta)=0## Right?- Frostman
- Post #3
- Forum: Advanced Physics Homework Help
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Charge invariance with Heaviside's function
I followed a demonstration in one of my electromagnetism books, but it is not clear to me. My problem is at the starting point. The book begins by considering the office defined in the following way: $$Q=\int d^4xJ^\alpha(x)\partial_\alpha\theta(\eta_\beta x^\beta)$$ where...- Frostman
- Thread
- Charge Function Heaviside function Invariance
- Replies: 17
- Forum: Advanced Physics Homework Help
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Conservation of charge with Dirac delta
So that factor ##3## really isn't there, because there's ##\sum_n## in front of everything, right?- Frostman
- Post #4
- Forum: Advanced Physics Homework Help
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Conservation of charge with Dirac delta
Hello, I was reviewing a part related to electromagnetism in which the charge and current densities are defined by the Dirac delta: ##\rho(\underline{x}, t)=\sum_n e_n \delta^3(\underline{x} - \underline{x}_n(t))## ##\underline{J}(\underline{x}, t)=\sum_n e_n \delta^3(\underline{x} -...- Frostman
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- Charge Charge density Conservation Conservation of charge Continuity equation Current density Delta Dirac Dirac delta
- Replies: 5
- Forum: Advanced Physics Homework Help
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De-excitation of a moving atom with photon emission
I tried, but the more I go I get lost in the accounts. I'm not even rewriting what I wrote here on the forum because it seems to me just a waste of time, but to show that I tried to do the math I am attaching the spreadsheets. As this is an exam to be done along with 2 exercises in 2 hours...- Frostman
- Post #3
- Forum: Advanced Physics Homework Help
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De-excitation of a moving atom with photon emission
The information I have are the following: ##p^\mu=(E, p, 0, 0)## ##p'^\mu=(E', p'\cos\beta, -p'\sin\beta,0)## ##k^\mu=\tilde{E}(1, \cos\alpha, \sin\alpha, 0)## Where: ##E=\sqrt{M^2+p^2}## ##E'=\sqrt{m^2+p'^2}## Using the conservation of the four-momentum ##p^\mu=p'^\mu+k^\mu##...- Frostman
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- Atom Conservation of energy Emission Four momentum Photon Photon emission Special relativity
- Replies: 6
- Forum: Advanced Physics Homework Help
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Magnetic field generated by a current in a wire - special relativity
First I wrote in ##S'##, by using Gauss theorem $$ \int_{\Sigma} \underline E' \cdot \hat n d\Sigma = \frac Q {\varepsilon_0} \rightarrow E'(r)2\pi rH=\frac{\lambda'H}{\varepsilon_0} $$ $$ \underline E'(\underline r)=\frac{\lambda'}{2\pi\varepsilon_0r}\hat r $$ Its components are...- Frostman
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- Charge density Current Current density Elecrtomagnetism Field Magnetic Magnetic field Relativity Special relativity Wire
- Replies: 1
- Forum: Introductory Physics Homework Help
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Constant acceleration in a rocket
Okay, it's an hyperbola. Furthermore, the more the acceleration value is greater, the more the trend is that of: ##x(t)=|t|## and this one is the trend of the light signal. The two trends, as I have drawn them, never meet.- Frostman
- Post #5
- Forum: Introductory Physics Homework Help