particle physics: status and perspectives part 9: energy frontier and open questions manfred jeitler

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Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

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Page 1: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

Particle Physics: Status and PerspectivesPart 9: Energy Frontier and Open Questions

Manfred Jeitler

Page 2: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

Supersymmetry

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Page 3: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

Supersymmetry

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Every fundamental matter particle should have a massive "shadow" force carrier particle, and every force carrier should have a massive "shadow" matter particle.

This relationship between matter particles and force carriers is called supersymmetry.

For example, for every type of quark there may be a type of particle called a "squark."

Page 4: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

Supersymmetry (“SUSY”)

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Page 5: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

Cancellation of quadratic terms (divergences)

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to avoid quadratic divergences in Higgs mass, “fine-tuning” is needed

Page 6: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

Running Coupling constants: Grand Unification

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U(1) (hypercharge) SU(2) (left) SU(3) (color) coupling constants get almost equal at high energies but not quite, in Standard Model (left) perfect match in Supersymmetry (right)

Page 7: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

Parameters of the Standard Model

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α1 = (5/3)g′2 /(4π) = 5α/(3 cos2 θW )

α2 = g2/(4π) = α/ sin2 θW

α3 = gs2/(4π)

α1(MZ) = 0.017

α2(MZ) = 0.034

α3(MZ) = 0.118 ± 0.003.

Page 8: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

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massive astrophysical cosmic halo objects?weakly interacting massive particles?

questions of cosmology to particle physics:Why is there more matter than anti-matter in the universe?What is the universe made of? What is dark matter?What is dark energy?

answers to these questions concerning the largest scales might come from the physics of the smallest scales - elementary particle physics

dark matter: MACHOS vs WIMPS

Page 9: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler
Page 10: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

How to see SUSY decays

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SUSY particles may show very clear signatures due to cascade decays

Page 11: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

11LIGO (Laser Interferometer Gravitational Wave Observatory, USA)

measurement of gravitational waves

Page 12: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

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important questions of today’s particle physics(ongoing experiments)

• Why are particle masses so different?

• Is there an overall (hidden) symmetry such as supersymmetry (SUSY) “mirror world” of all known particles?.

• What is the nature of “dark matter” and “dark energy” in the universe?

• Why is there more matter than anti-matter?

• Why have neutrinos such small mass?

• Is there a Grand Unification which combines all interactions, including gravitation?

• Are there extra dimensions, D > 4 ? ( string theory, …)

Page 13: Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler

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