Presentation is loading. Please wait.

Presentation is loading. Please wait.

Task E - A0 and related activities

Similar presentations


Presentation on theme: "Task E - A0 and related activities"— Presentation transcript:

1 Task E - A0 and related activities
A.C.MELISSINOS Faculty S.VORONOV Res. Assoc. (2003) R.TIKHOPLAV Graduate Students S.SELETSKIY W.BUTLER --- NLC SOURCE DEVELOPMENT --- LASER ACCELERATION EXPERIMENT ELECTRON COOLING OF ANTIPROTONS IN RECYCLER A0 PHOTOINJECTOR (FERMILAB) SEARCH FOR COHERENT BACKGROUND FIELDS (proposed) PHENOMENOLOGY 9/18/2018 Task E/DOE review/ACM

2 A0 (FNPL) PHOTOINJECTOR
--- Train of 800 pulses spaced µs --- Charge per pulse > 1 nC --- Emittance ~ -mm-mr --- Pulse length < 1 ps Can be operated remotely from LBL, DESY EXPERIMENTS: Generation of flat beams --- Beam diagnostics for ultra-short pulses --- Plasma wakefield acceleration                                             Rochester built and operates/maintains/improves the injection laser 9/18/2018 Task E/DOE review/ACM

3 TEM01* (DOUGHNUT-SHAPE) MODE
Nd:glass laser with wavelength =1054 nm is used; compressed and amplified it will deliver 1J in 1ps pulse The laser operates in the TEM01 mode Radial polarization (TEM01* mode) is used for symmetry reasons and to gain a factor of 2 in accelerating field 9/18/2018 Task E/DOE review/ACM

4 15 MeV 50 MeV 150 MeV 9/18/2018 Task E/DOE review/ACM

5 ELECTRON COOLING Electron Energy 3.5 MeV Electron Current 500 mA
Cooling section length m Preserve electron beam focussing by using longitudinal magnetic field Gauss Tolerance on transverse field Gauss Tolerance on beam loss < 2% 9/18/2018 Task E/DOE review/ACM

6 9/18/2018 Task E/DOE review/ACM

7 The angular spread of the beam must be less than 10-4 radians
Uncompensated field Compensated field The angular spread of the beam must be less than radians 9/18/2018 Task E/DOE review/ACM

8 DETECTION OF COHERENT FIELDS
Possibilities: Coherent axion field Dilaton field Quintessence field  +   -  In the LIGO interferometer  = 2(3x1014) is resonant; if  ±  is also resonant, The SIDEBANDS build up EXAMPLE: Coherent axion field h = 10-20 LIGO sensitivity h = 10-23 9/18/2018 Task E/DOE review/ACM

9 Response of the LIGO interferometer to a coherent
high frequency wave incident at an angle of 30° The first peak is at kHz 9/18/2018 Task E/DOE review/ACM

10 9/18/2018 Task E/DOE review/ACM

11 NEUTRINO SCATTERING IN A MAGNETIC FIELD Yaroslav University (2003)
K.S.McFarland, A.C.Melissinos, N.V.Mikheev and W.W.Repko Yaroslav University (2003) ν + B → ν + γ (high energy) Conversion probability for 50 GeV neutrinos When B = 2.2 T L = 10 m 9/18/2018 Task E/DOE review/ACM

12 “RUNNING” OF THE GRAVITATIONAL COUPLING CONSTANT
Solid line Classical Evolution Dotted line Unification with the Gauge couplings 9/18/2018 Task E/DOE review/ACM

13 Supplementary slides 9/18/2018 Task E/DOE review/ACM

14 9/18/2018 Task E/DOE review/ACM

15 9/18/2018 Task E/DOE review/ACM

16 Beam recirculation experiment with U-bend beam line
Multiple improvements let us to demonstrate stable recirculation of 0.5 A electron beam Better understanding of beam optics and improvements in the gun and collector design made it possible to recirculate a beam of up to 1.7 A at 3.5 MV for several minutes – it’s 6 MW of beam power! Beam recovery after an interruption of a 1-A beam recirculation The use of a protection system, allowing to shut the gun off during interruptions, helped to avoid large drops of the Pelletron voltage and large pressure jumps. As a result, the beam recovery time is as low as 15 seconds 9/18/2018 Task E/DOE review/ACM

17 Cooling section Parameter Value Units Number of solenoids 10 Length of solenoids 190 cm Working magnetic field G Maximal magnetic field 200 Solenoid current 4 A Coefficient of the shielding of solenoids 1000 Gap length 8 Number of gap correctors 20 Number of transverse field correctors per solenoid Requirements on the magnetic field in the cooling section Beam angular spread in the cooling section should be less than 10-4 rad. This requirement impose certain restrictions on the quality of the magnetic field in the cooling section. longitudinal field transverse field To cancel the solenoid edge effect electron at the entrance of the cooling section should have a proper angular momentum. To impart an angular momentum onto the electron beam the electron gun is immersed in a solenoidal magnetic field. Thus, a beam is produced by a 5-mm diameter cathode in a 600-G magnetic field and then propagated to the cooling section, where it is injected into a 150-G solenoid. Algorithm of field correction was used to set the field of required properties Simulation of electron’s motion in uncompensated magnetic field Simulation of electron’s motion in the compensated magnetic field 9/18/2018 Task E/DOE review/ACM

18 9/18/2018 Task E/DOE review/ACM

19 9/18/2018 Task E/DOE review/ACM


Download ppt "Task E - A0 and related activities"

Similar presentations


Ads by Google