Role of Exclusion principle in formation of black holes.

aaryan0077
Messages
69
Reaction score
0
I was reading something about formation of black hole, and it was given that exclusion principle has a role in BH (Black Hole) formation.
It read "when star become small, the matter particle get very near each other, and so acc. to Pauli's Exclusion principle they must have different velocities. This makes them move away from each other and star expand, and remains at constant radius, by balance btw this force from repulsion and attraction by gravity."

But exclusion principle says about spin, and its uncertainty principle that deals in velocity and position, so is not it that it should be like "... acc. to Uncertainty Principle..." and not "... acc. to Pauli's Exclusion Principle".

Or I don't know the role of Exclusion principle in BH formation, or it that really uncertainty principle that plays a role in shaping the formation of BH.
Please help me out. I am totally confused.
 
Physics news on Phys.org
Thread 'Can this experiment break Lorentz symmetry?'
1. The Big Idea: According to Einstein’s relativity, all motion is relative. You can’t tell if you’re moving at a constant velocity without looking outside. But what if there is a universal “rest frame” (like the old idea of the “ether”)? This experiment tries to find out by looking for tiny, directional differences in how objects move inside a sealed box. 2. How It Works: The Two-Stage Process Imagine a perfectly isolated spacecraft (our lab) moving through space at some unknown speed V...
Insights auto threads is broken atm, so I'm manually creating these for new Insight articles. The Relativator was sold by (as printed) Atomic Laboratories, Inc. 3086 Claremont Ave, Berkeley 5, California , which seems to be a division of Cenco Instruments (Central Scientific Company)... Source: https://www.physicsforums.com/insights/relativator-circular-slide-rule-simulated-with-desmos/ by @robphy
In Philippe G. Ciarlet's book 'An introduction to differential geometry', He gives the integrability conditions of the differential equations like this: $$ \partial_{i} F_{lj}=L^p_{ij} F_{lp},\,\,\,F_{ij}(x_0)=F^0_{ij}. $$ The integrability conditions for the existence of a global solution ##F_{lj}## is: $$ R^i_{jkl}\equiv\partial_k L^i_{jl}-\partial_l L^i_{jk}+L^h_{jl} L^i_{hk}-L^h_{jk} L^i_{hl}=0 $$ Then from the equation: $$\nabla_b e_a= \Gamma^c_{ab} e_c$$ Using cartesian basis ## e_I...
Back
Top