Ion Beam Intensity Enhancement Through Electron Heating in Collider Experiments

 
Electron heating of the ions in the Collider
V. Parkhomchuk
BINP Novosibirsk
29 M|ay 10+5 minutes
 
XI Session of the NICA MAC, May 27-29
, ОИЯИ
Online sesiion from BINP
 
 
e
Z
i
-
charge of ion
 
Classical radius
 
R average radius of collider                      bunch length  
    
emitance
 
 
Electron heating- High initial intensity- fast losses,
proton beam current afte start electron cooling
From 0.73 go to 0.25 mA!
100-300 s-  Laslet tunr near 0.1-0.2, equilibrium
  t>300 s Intra Beam Scatering
 
Fig 1. COSY low energy (200 MeV) proton
beam cooling current (0.2A)
 
Laslet tune shift
 
Fig.2  SIS-18 accumulation
krypton ion beam
After 2 mA started
oscillations at ion beam
end acculamution decreseed,
after 5 mA   stopped-
As results high losses
between new injection are
equal adding new portion
ions.
 
 
Fig
 
3
. 
 Acselleration
 and them electron cooling proton beam
with energy 400 MeV, proton beam with energy 400 MeV
.
The top lines show 
 proton beam current mA (black without modulation of
the energy electron beam red line with 300 V modulation of energy (potential cathode)) 
В
The down lines proton beam sizes  mm (sigma,x,y)
,
 
 
       
Fig.4 Losses rate 
 versus proton beam carrent
dI/dt/I (
Ep=400 
МэВ, 
Jecooling=600ma)
.
 for different energy modulation  0,200,300 V
 
where me is the electron mass, c is the
speed of light, re is the classical radius of
the electron, ne is the electron beam
density , ln (
max

min) is the Coulomb
logarithm of collisions. Electrons passing
by particles scatter on it and lead to the
heating of its momentum at a speed
       
Maximum ion beam intensity with electron cooling
 
Cooling force
 
Losses energy the ion by excitation
electrons moving  (cooling)
 
 
 
 
Heating from thermal mooving
electrons
 
 
In equilibrium temperatures are equal
But heavy ions moved very slowly
 
For high the ion beam density at interaction regions many
fluctuation from other ions
 
 
Heating from others ions should be
less electron cooling
 
4.6 GeV/n     Ni<8E10
0.5 GeV/n    Ni<5E8
 
b
e
a
m
-
p
l
a
s
m
a
i
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s
t
a
b
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l
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t
y
,
 
b
e
a
m
i
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,
 
o
r
 
b
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m
p
-
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-
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n
s
t
a
b
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l
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t
y
 
 
Plasma model of instability
 
Slowly moved ion and electrons  fast compensated
 return electric field  for ion plasma oscilation. It means the mplitude
Of oscillation can increase.
 
Increasing space charge oscilation
after passing  cooling section
 
Det(A) <1  cooling,   Det(A)>1 heating
 
 
CONCLUSION
1-
 
 Electron cloud effects are problems for
electron positron collider. Small solenoids in
collider help control this effect
2- Ion beams with electron cooling system
should care for limited heating
3- Hollow electron beam are one of the ways for
decreasing  unlikely interaction
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The study discusses electron heating of ions in collider experiments at the Collider V. ParkhomchukBINP facility in Novosibirsk. It explores the effects of electron cooling on ion beams, ion beam oscillations, losses, and ion beam intensity enhancement. Various factors such as ion charge, classical radius, cooling mechanisms, beam currents, and energy modulations are analyzed to optimize ion beam performance. Experimental results and theoretical calculations provide insights into maximizing ion beam intensity through effective electron heating strategies.

  • Ion Beam
  • Electron Heating
  • Collider Experiments
  • Beam Intensity Enhancement
  • ParkhomchukBINP

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  1. Electron heating of the ions in the Collider V. Parkhomchuk BINP Novosibirsk 29 M|ay 10+5 minutes XI Session of the NICA MAC, May 27-29, Online sesiion from BINP

  2. ??=(???)2 ???2 eZi-charge of ion Laslet tune shift Classical radius N r R = i i emitance ?? R average radius of collider bunch length 2 3 l b COSY 200 MeV proton beam 10 10 Electron heating- High initial intensity- fast losses, proton beam current afte start electron cooling From 0.73 go to 0.25 mA! 100-300 s- Laslet tunr near 0.1-0.2, equilibrium t>300 s Intra Beam Scatering i r dt p 8 Cj 1 Cj 2 6 Cj 3 10 Cj 4 100 4 2 2 4 1 N cLn dp = i c 2 2 0 3 2 / 3 2 / 1 2 0 0 0 100 200 300 400 500 600 0 Cj 0 551 time sec horizontal sigma /1mm vertical sigma /1mm proton beam current /(0.1mA) electron beam current /100mA Fig 1. COSY low energy (200 MeV) proton beam cooling current (0.2A)

  3. 6 34+ current Kr signal pickup electrodes Fig.2 SIS-18 accumulation krypton ion beam After 2 mA started oscillations at ion beam end acculamution decreseed, after 5 mA stopped- As results high losses between new injection are equal adding new portion ions. ion beam current (mA) 4 2 0 10 20 30 40 time (s)

  4. 0,010 no modulation 200 V modulation 300 V modulation CELSIUS (1999) 400 MeV pbeam Je=600 mA beam current no modulation beam current 300 V modulation electron energy pbeam r.m.s. size (mm) pbeam r.m.s. size (mm) with 300 V modulation losses rate dI/dt/I (1/s) 8 0,005 7 Proton beam current (mA) 6 5 4 0,000 0 1 2 3 4 5 6 3 proton beam current (mA) Fig.4 Losses rate versus proton beam carrent dI/dt/I (Ep=400 , Jecooling=600ma). for different energy modulation 0,200,300 V 2 1 0 -1 0 50 100 150 time (s) Fig 3. Acselleration and them electron cooling proton beam with energy 400 MeV, proton beam with energy 400 MeV. The top lines show proton beam current mA (black without modulation of the energy electron beam red line with 300 V modulation of energy (potential cathode)) The down lines proton beam sizes mm (sigma,x,y),

  5. Maximum ion beam intensity with electron cooling n Z e F eff 2 4 ) / ln( 4 V mV eff n Z e dt 4 2 4 ln( / ) = max min V i e 3 Cooling force mV n e where me is the electron mass, c is the speed of light, re is the classical radius of the electron, ne is the electron beam density , ln ( max min) is the Coulomb logarithm of collisions. Electrons passing by particles scatter on it and lead to the heating of its momentum at a speed e Z Losses energy the ion by excitation electrons moving (cooling) = 2 max min FV i 3 4 2 2 4 ln( / ) dp = Heating from thermal mooving electrons max min i e V eff m In equilibrium temperatures are equal But heavy ions moved very slowly V = 2 2 eV eff M For high the ion beam density at interaction regions many fluctuation from other ions 4 N = * 3 max in 3 Heating from others ions should be less electron cooling M 2 ( F 2 ) * N FV

  6. 6 = 2 2 4 2 i 2 e 4 4 rc r n 4 c r n 1 i i e e ln( / ) max min 4 6 6 1 . 1 17 6 10 / 1 ( ) n n cm ilab elab 4 cool 2 4 ( ) ln( / ) l r r min i e 4.6 GeV/n Ni<8E10 0.5 GeV/n Ni<5E8 beam-plasma instability, beam instability, or bump-on- tail instability

  7. Plasma model of instability proton and electron beam position (cm) 140 proton electron 1,0 120 interaction at zone +-125 cm 100 electic field (V/cm) 80 60 0,5 40 20 0 -20 0,0 -40 -300 -200 -100 0 100 200 300 -200 -100 0 100 200 position along cooling section (cm) position along cooling section (cm) Slowly moved ion and electrons fast compensated return electric field for ion plasma oscilation. It means the mplitude Of oscillation can increase.

  8. Increasing space charge oscilation after passing cooling section Det(A) <1 cooling, Det(A)>1 heating

  9. CONCLUSION 1- Electron cloud effects are problems for electron positron collider. Small solenoids in collider help control this effect 2- Ion beams with electron cooling system should care for limited heating 3- Hollow electron beam are one of the ways for decreasing unlikely interaction

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