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group_secar2.0

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Group SECAR2.0

– by Alex, Nadeesha and Louis –

DAY1

Getting started

Choosen example reaction: 45V(p,γ)46Cr
⇒important for 44Ti production rate in core collapse Supernova (Horoi et al. Nucl.Phys.A 718, (2003))
Beam: 45V13+ of 135 MeV (1% enegry spread)

Understanding COSY Matrix output

Command: OV 1 1 0 ; {order 1, phase space dim 1 INCLUDING ENERGY, # of parameters 0}
Output:

1.00.00.00.0-0.41
2.21.00.00.0-0.35

Explanation:

R11R120.00.0R15
R21R220.00.0R25

R11 = 1.0 is “Magnification”, i.e. no magnification provided with the dipole.
R12 = 0.0 is “Focusing”, i.e. no focusing is provided by the dipole.
R21 = 2.2 is approximate “Path length”,which is 0.5+0.78+1.0 meters
R22 = 0.0 mean that output angles does not depend on input angles.
R15 = -0.41 is ToF difference due to different initial position.
R25 = -0.35 is ToF difference due to different initial angle.

Reaction Kinematics Calculation

Reaction summary for 45V+p→γ+46Cr, Ekin(45V)=135 MeV
The maximum γ energy is 8.481 MeV. The minimum γ energy is 7.249 MeV.
The maximum 46Cr energy is 132.634 MeV. The minimum 46Cr energy is 131.402 MeV. The maximum 46Cr angle is 0.13 degrees.

If we assume a normalized emittance of 0.6 π mm mrad provided from ReA3 at 3.0 MeV/u the geometric emittance is 0.6/0.08 = 7.5 π mm mrad.
With the spot size on the target, designed to be ±0.5 mm (1σ), the anglular spread then is ±15 mrad.
Adding the calculated spread from the reaction with the target of 0.13 deg = ±2.26 mrad we get ±17.26 mrad of angular spread.
⇒COSY beam input: SB 0.0005 0.01726 0 0.0005 0.01726 0 0 0.0047 0 0 0 ;
Output for this beam passing the dipole:

DAY2

Emittance Measurement

The distance between the center of Q7 and the focal plane FP2 is 6.085 m as extracted from the script file.

Quadrupole strenght variations for emittance measurment

BQ7 [T] Xmax[m] ap [m] Bρ* [Tm] L [m] K
0.02 2.91E-03 0.13 0.8 6.085 0.065384615
0.01 2.27E-03 0.13 0.8 6.085 0.032692308
0 1.62E-03 0.13 0.8 6.085 0
-0.01 1.20E-03 0.13 0.8 6.085 -0.032692308
-0.02 9.08E-04 0.13 0.8 6.085 -0.065384615
-0.03 6.23E-04 0.13 0.8 6.085 -0.098076923
-0.04 9.54E-04 0.13 0.8 6.085 -0.130769231
-0.05 1.60E-03 0.13 0.8 6.085 -0.163461538
-0.06 2.26E-03 0.13 0.8 6.085 -0.196153846

*Bρ the magnetic rigidity was extracted from COSY by comand CONS(CHIM)

Fit of the data to parabola

Fit result for parabola Xmax2 = σ11 = a·K2 - 2ab·K + ab2 + c is:

a = 0.000362572706
b = 0.0834414129893
c = 3.506973286e-07

The consistency check for beam size calculation in Q7 shows:
X_calculated = 3.13mm, X_cosy_read_out = 3.16mm at the Q7 exit.
Emittance calculated from fit parameters ε= √(ac) / L2 = 3.05E-7 π m rad = 0.305 π mm mrad.
Start beam emittance= XX · AX= 0.2 π mm mrad, so the emittance grows from the start to the focal point.
This emittance grow is possibly due to the optics aberrations. That is because the input COSY file does a 4th-order-calculation. Also the measured points don't fit the parabola ideally, i.e. the optics is non-linear.

DAY3

Impact of Lenght Change in Quadrupole 2

The effective length of Q2 was reduced by 3% to 0.291m with the drift lenghts before and after increased by 0.0045m.
This led to a mass resolution change from 445 to 102 for the standard particle of the script.

/srv/thewikis/JIOSS/data/attic/group_secar2.0.1536778433.txt.gz · Last modified: 2018/09/12 14:53 by plastun