Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 Synchrotron radiation in LHC: spectrum and dynamics The Large Hadron Collider (LHC)

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Presentation transcript:

Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 Synchrotron radiation in LHC: spectrum and dynamics The Large Hadron Collider (LHC) will collide 7 TeV protons in the same tunnel (circumference 27 km) where the Large Electron Project (LEP) operated with 100 GeV electrons. Assuming for simplicity the same bending radius in dipole magnets of 2900 m, calculate the following synchrotron radiation parameters for the three cases: for protons at the injection energy of 450 GeV, at the design energy of 7 TeV and for the electrons at 100 GeV:  typical (‘critical’) photon energy of emitted synchrotron radiation  energy loss per turn  the damping times for energy and transverse oscillations The proton mass is GeV and the electron mass is MeV

Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 Future Circular Collider (FCC) New superconducting materials may allow in the future to build 20 Tesla dipole magnets. Assuming 10 km bending radius (about 100 km long tunnel, 2/3 filled with dipoles)  To what maximum energy will FCC be able to accelerate protons?  What will be the typical photon energy emitted by protons and what will be the energy loss per turn?  Estimate the damping time and the equilibrium emittance of the protons stored at the top energy

Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 Synchrotron light source that never was: LEP at 5 GeV The equilibrium electron beam emittance at 100 GeV at LEP was about 0.06 mm·mrad. If we tried to operate LEP at 5 GeV, how small an emittance could one hope to achieve using the same lattice? What would be the damping time at this energy (a few milliseconds at 100 GeV)? Find the length of wiggler magnets you would need to install in the straight sections of the ring (assume wiggler field of 2 Tesla), in order to reduce the damping times at 5 GeV by a factor of 1000.

Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 High Energy options: 100 km tunnel? 50 TeV c.o.m. with 8.3 T LHC type dipoles 100 TeV c.o.m. with 16 T 120 TeV c.o.m with 20 T

Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014

Synchrotron radiation power Power emitted is proportional to: Energy loss per turn:

Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 Typical frequency of synchrotron light Due to extreme collimation of light observer sees only a small portion of electron trajectory (a few mm) Pulse length: difference in times it takes an electron and a photon to cover this distance

Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014

Synchrotron radiation in LHC The critical photon energy is: The energy lost per turn in LHC at 7 TeV is about 7 keV, while at LEP it was 3 GeV The damping times will be on the order of 1 day at LHC and a few milliseconds at LEP. 450 GeV7000 GeV100 GeV electrons Relativistic  ‘000 cc 0.01 eV42 eV0.8 MeV

Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 FCC compared to LHC The magnetic rigidity at 20 Tesla and radius of 10’000 meters reaches 200’000, the beam energy will be then 60 TeV The critical photon energy is proportional to the cube of energy and inversely proportional to the bending radius Energy loss per turn will be almost 1500 times higher, or 10 MeV Damping times will be about 2 seconds

Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 Synchrotron light source: LEP at 5 GeV The equilibrium emittance scales as square of the storage ring energy, so at 5 GeV the emittance could be 400 times smaller, i.e nm·rad! The damping times on the other hand scale as the cube of ring energy and would become very long indeed: 24 and 48 seconds. With wigglers in LEP at 5 GeV, the total radiation loss per turn: where then and the required length is