Beam Conditions and Effects in Particle Physics Experiments
All needed information is in the EIC CDR
https://www.bnl.gov/ec/files/EIC_CDR_Final.pdf
specifically in section 3.1 and tables 3.3 to 3.5 and section 3.2
detector solenoid aligned with the lepton beam
8 mrad
reduction of synchrotron radiation
electron beam displacement at the end of the solenoid would be too big to handle
E.C. Aschenauer
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electron beam
p/A beam
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Low luminosity
more challenging Beam dynamics
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Size of crab angle directly impacts angular opening of the first forward spectrometer
dipole B0 (polar angle)
Impact on main detector acceptance
beams not back to back
solenoid aligned
with electron beam
very small charged particle bending on one side of the
outgoing hadron beam line
poor momentum resolution (and a strong functional
azimuthal asymmetry of the acceptance at high
)
transverse vertex (x-direction) is depending on what collisions ones has head head
vs. tail-tail
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bring focusing magnets close to IP
no separator dipole
reduce detector background
reduced SR
beams less in one common beam pipe
Multi-staged separation
separate beam
from particles needed for physics
space for forward equipment along beam line
E.C. Aschenauer
E.C. Aschenauer
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Angular “spread” of the beam away from
the central trajectory.
Gives some small initial transverse
momentum to the beam particles
impact on p
T
resolution
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beam energy is a gaussian centered on
value i.e 5 GeV, with a RMS ~10
-4
GeV
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both beams have a longitudinal extension
hadron beam < 10 cm & electron beam
~1cm
E.C. Aschenauer
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Rotate the ESR reference plane about a line through IP6 and IP8 by ~200
µRad
for IP-6 this means a vertical shift of 1.521mm at the end of b2er
(z=14998.27mm), that makes it a about 100
rad angle
very small angle should be not to critical for science
1022.3 m
Rotate ESR Plane about line through
IP6 and IP8 by ~200 µR
ESR elevation at IR 6 & IR8 = 1270
mm
510.8 m
ESR elevation at IR4 & IR10 = 1168
mm
(low by 102 mm)
ESR elevation at IR2 & IR12 = 1066
mm
(low by 204 mm)
X
Z
All the effects from before
angular beam divergence
beam energy spread
bunch length
crossing angle and crab cavities
•
Roman pot detectors need to sit before the crab cavities to avoid decorrelation of
forward scattered protons and IP info
E.C. Aschenauer
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RMS hadron bunch length ~10cm.
Because of the rotation, the Roman Pots see the bunch crossing smeared in x.
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Looking along the
beam with no
crabbing.
~1.25mm
E.C. Aschenauer
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~20 cm
High Divergence
High Acceptance
Acceptances: Beam-pipe and Magnet apertures
low p
T
- Acceptance: normalized beam emittance and beta function
10
separation RP to beam
E.C. Aschenauer
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Critical accelerator and beam conditions for E.C. Aschenauer's physics research at BNL are discussed, including effects on the main detector, consequences of crossing angle adjustments, important particle beam parameters, and the rotation of the ESR reference plane. Detailed information on beam divergence, energy spread, bunch length, and ESR elevation changes is provided.
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Presentation Transcript
Accelerator and Beam conditions critical for physics E.C. Aschenauer (BNL) Office of Science
Effects to be considered for the Main Detector All needed information is in the EIC CDR https://www.bnl.gov/ec/files/EIC_CDR_Final.pdf specifically in section 3.1 and tables 3.3 to 3.5 and section 3.2 Backward electron beam p/A beam Forward detector solenoid aligned with the lepton beam 8 mrad reduction of synchrotron radiation electron beam displacement at the end of the solenoid would be too big to handle 2 E.C. Aschenauer
Consequences of Crossing Angle Crossing angle of 25 mrad bring focusing magnets close to IP no separator dipole reduce detector background reduced SR beams less in one common beam pipe Multi-staged separation separate beam from particles needed for physics space for forward equipment along beam line However, crossing angle causes Low luminosity more challenging Beam dynamics avoided by Crab Crossing Impact on Physics: Size of crab angle directly impacts angular opening of the first forward spectrometer dipole B0 (polar angle) Impact on main detector acceptance beams not back to back solenoid aligned with electron beam very small charged particle bending on one side of the outgoing hadron beam line poor momentum resolution (and a strong functional azimuthal asymmetry of the acceptance at high ) transverse vertex (x-direction) is depending on what collisions ones has head head vs. tail-tail 3 E.C. Aschenauer
Important particle beam parameters Angular beam divergence Angular spread of the beam away from the central trajectory. Gives some small initial transverse momentum to the beam particles impact on pT resolution Beam Energy spread beam energy is a gaussian centered on value i.e 5 GeV, with a RMS ~10-4 GeV Bunch length both beams have a longitudinal extension hadron beam < 10 cm & electron beam ~1cm E.C. Aschenauer 4
Rotate eSR Rotate the ESR reference plane about a line through IP6 and IP8 by ~200 Rad for IP-6 this means a vertical shift of 1.521mm at the end of b2er (z=14998.27mm), that makes it a about 100 rad angle very small angle should be not to critical for science 1022.3 m ESR elevation at IR2 & IR12 = 1066 mm (low by 204 mm) 510.8 m X Z ESR elevation at IR4 & IR10 = 1168 mm (low by 102 mm) Rotate ESR Plane about line through IP6 and IP8 by ~200 R ESR elevation at IR 6 & IR8 = 1270 mm E.C. Aschenauer 5
Effects to be considered for the Forward Detectors All the effects from before angular beam divergence beam energy spread bunch length crossing angle and crab cavities Roman pot detectors need to sit before the crab cavities to avoid decorrelation of forward scattered protons and IP info ~1.25mm Looking along the beam with no crabbing. RMS hadron bunch length ~10cm. Because of the rotation, the Roman Pots see the bunch crossing smeared in x. Vertex smearing = 12.5mrad (half the crossing angle) * 10cm = 1.25 mm If the effective vertex smearing was for a 1cm bunch, we would have .125mm vertex smearing. 6 E.C. Aschenauer
Effects to be considered for the Forward Detectors Acceptances: Beam-pipe and Magnet apertures low pT - Acceptance: normalized beam emittance and beta function 10 separation RP to beam ??,?= ??,???/? High Divergence: smaller ? at IP, but bigger (z=30m) higher lumi., larger beam at RP High Divergence High Acceptance High Acceptance: larger ? at IP, smaller ?(? = 30?) lower lumi., smaller beam at RP ~20 cm E.C. Aschenauer 7
8 E.C. Aschenauer
