It stays for very long RG-time almost on the scaleless trajectory only to branch off into the broken phase
9/ 11
It stays for very long RG-time almost on the scaleless trajectory only to branch off into the broken phase
9/ 11
They correspond to the three different options for the Higgs mass term mu^2<0, mu^2=0 and mu^2>0
The mu^2>0 branch corresponds to the SM in which the electroweak gauge symmetry remains unbroken
6/11
They correspond to the three different options for the Higgs mass term mu^2<0, mu^2=0 and mu^2>0
The mu^2>0 branch corresponds to the SM in which the electroweak gauge symmetry remains unbroken
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But there is also a geometric interpretation that can be understood with little maths (but a lot of physics)
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But there is also a geometric interpretation that can be understood with little maths (but a lot of physics)
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6/7
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4/7
4/7
It explains radioactive alpha-decay where a whole Helium nucleus is emitted from a heavy decaying element even if the binding forces wouldn't allow this process classically
3/7
It explains radioactive alpha-decay where a whole Helium nucleus is emitted from a heavy decaying element even if the binding forces wouldn't allow this process classically
3/7
If you measure the position of the particle there is a finite probability it's outside the trap even if it never had enough kinetic energy to overcome the barrier. It 'tunnels' through the barrier
2/7
If you measure the position of the particle there is a finite probability it's outside the trap even if it never had enough kinetic energy to overcome the barrier. It 'tunnels' through the barrier
2/7
In classical mechanics you can know where a particle is and its momentum at the same time. In Quantum mechanics you can't. All information is in the wavefunction. Even if a particle is trapped, part of the wavefunction..
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In classical mechanics you can know where a particle is and its momentum at the same time. In Quantum mechanics you can't. All information is in the wavefunction. Even if a particle is trapped, part of the wavefunction..
🧵1/7
Until barely a century ago, no human ever knew whether there was more than one galaxy in the Universe. Think about that!
Until barely a century ago, no human ever knew whether there was more than one galaxy in the Universe. Think about that!
In the plot below we were at the blue, we are now at the red and could be as sensitive as the green markers
6/6
In the plot below we were at the blue, we are now at the red and could be as sensitive as the green markers
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4/6
Intriguingly, CMS, another experiment at the Large Hadron Collider, has also measured this process and sees the same anomaly, too
2/6
Intriguingly, CMS, another experiment at the Large Hadron Collider, has also measured this process and sees the same anomaly, too
2/6
Previous results disagreed with the Standard Model prediction for the branching fraction and angular distribution
The new measurement has almost twice as much data and still disagrees!
🧵1/6
Previous results disagreed with the Standard Model prediction for the branching fraction and angular distribution
The new measurement has almost twice as much data and still disagrees!
🧵1/6
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Again, the bar on the right part is the line connecting the two particles
8/14
Again, the bar on the right part is the line connecting the two particles
8/14
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While R^2 is simply connected (every loop can be contracted to a dot), this space is not
4/14
While R^2 is simply connected (every loop can be contracted to a dot), this space is not
4/14
Two loops that can be continually transformed into each other are equivalent. But because the tip of the cone is missing, any number of rotations around the cone can't be transformed into one with fewer or more windings
3/14
Two loops that can be continually transformed into each other are equivalent. But because the tip of the cone is missing, any number of rotations around the cone can't be transformed into one with fewer or more windings
3/14