Linac96

SECONDARY ELECTRON MONITOR FOR ELECTRON BUNCH PHASE DISTRIBUTION MEASUREMENT WITH SUBPICOSECOND RESOLUTION

A.M.Tron, I.G.Merinov

MEPhI, Kashirskoe sh. 31, 115409 Moscow, Russia

Abstract

Secondary electron monitor using longitudinal rf-modulation of low energy secondary electrons, with initial energy in eV range, for bunch phase distribution measurement of electron linac bunches with subpicosecond resolution is considered. Analysis of limiting resolution for this method, construction particularities of the monitor, and specific example of its design for the measurement of the TTF linac beam will be presented.

Introduction

Development of electron linacs demands creation of a bunch length monitor with subpicosecond resolution that is equivalent to the measurements in frequency domain up to 1 THz or in submillimetre wave range. The monitor has to be compacted, selfcalibrating, unpertubing a beam, compatible with UHV, radiation resistive.

Several approaches are known for solving this challenge. One of them consists in estimation of the rms bunch length through two beam current harmonics assuming, for example, bunch charge distribution is Gaussian [1] or using single harmonic [2] closed to the rms frequency of a beam spectrum where its amplitude is most sensitive to the bunch length changes. For the Gaussian bunch the rms bunch length s can be determined from equation


where in, im are beam current harmonics unknown precisely. Hence, the technique needs some one to calibrate it.

Method of interferometry of coherent radiation and the others closed to it [3,4] are restricted by wave lengths being more than beam diameter or hole diameter of screen[5].

The use of incoherent radiation, for example, on a scheme: Cherenkov radiator plus a streak camera [6,7], is mainly limited due to the longitudinal chromatic aberration in the camera gap (photocathod - mesh distance) caused by initial velocity spread of photoelectrons. In plane-parallel geometry of the gap one can expect the limiting resolution till 1 ps [8].

In the paper the secondary electron monitor coming up to the above mentioned requirements more completely is presented. (The monitor based on the delta-rays is presented at this Conf. too)

It should be noted that in the best work [9] on research of time dispersion of SEM (the gap voltage was 3.6 kV) it was measured, in fact, its longitudinal chromatic aberration only, and the SEM time dispersion for metal is within 1...10 fs [12].

BPD monitor

Secondary electron monitor for bunch phase distribution (BPD) measurements with subpicosecond resolution is schematically shown in Fig.1.

Fig.1. Layout of BPD monitor (a) and geometry of its primary converter (b).

Here BPD of a primary beam (1) in a result of the beam interaction with a carbon fibre (2) under negative potential (U0) is isohronously transferred into the same distribution of secondary electrons which, then, is coherently transformed into transverse one in the plane of multichannel collector (6) through rf-modulation in the gap of toroidal resonator (3) and magnet (5) allowing direct presentation the BPD on a low frequency display. Taking into account that the beam diameter is rather small (of 1...2 mm) and the smaller h-distance the less time transport spread (of the electrons) the carbon target was placed from the resonator at small fixed distance h = 2 mm, and this monitor unit is moved in the beam for a time of measurements only.

The monitor phase resolution (Dj) is mainly defined by the time transport spread (Dj1) of the electrons on h-distance (2 mm), the shutter phase resolution (Dj2) [10] and the additional phase dilution (Djq) caused by the beam space charge effect. Then, considering the above mentioned quantities as the independences one can estimate Dj using known algorithm from [10].

Time transport spread in primary converter

Time transport spread of the secondaries (Dt) at their motion in the field of charged cylindrical electrode under potential -U0 on h-distance (Fig.1,b) until the conducting wall (A-A) was obtained by numerical simulation using relativistic equations and taking for the electrons emitted from carbon their initial energy and angular distributions from [11]. Results of this calculation are presented in Fig.2, where fW and ft are the initial energy distribution and temporal one in the plane A-A, respectively, for h = 5 mm, U0 = 8 kV and 2R0 = 0.1 mm. FWHM of ft is 0.227 ps that corresponds the time transport spread of two electrons with initial energies of 0.335 eV and 3.925 eV if they would move along the z axis.

Fig.2. Initial energy distribution of the secondary electrons (left) and their time distribution at the exit of primary converter at U0 = 8 kV, h = 5 mm (right).

In Fig.3,4 are shown the dependencies of the FWHM of ft (Dt) vs. the electrode radius and voltage, respectively.

Fig.3. Time spread of secondary electrons in the primary converter vs. the target radius (R0) for different distances h (see Fig.1.b) at U0 = 8 kV.

Fig. 4.

The case of very large R0 (more 100 mm at small h) corresponds the plane - parallel geometry similar to the accelerating gap (from a photocathod to mesh) in a streak camera [6,7]. One can see that using the plane - parallel geometry and voltage up to 20 kV and higher it is impossible to reach t = 1 ps or less at input electron size of more several tenth mm. These results are closed to one published in [8]. For our monitor R0 = 0.01 mm, U0 = 8 kV, h = 2 mm and t = 30 fs, i.e. 0.014° in deg. of 1.3 GHz.

Monitor resolution

Beam space charge effect is the main one limiting the monitor resolution. Dependencies of the additional phase dilution (Djq) and momentum spread (dq) caused by the effect vs. the target place relative to the beam axis are plotted in Fig.5 for the geometry of the primary converter mentioned above and for the next beam parameters: electron energy - 10 MeV; beam radius - 0.5 mm; bunch length in phase of 1.3 GHz - 1.5; bunch population - 3108. For calculation the ellipsoidal bunch with uniform density was taken. Charges induced by the beam on the target surface was not taken into account.

Fig.5. Electron phase dilution (2) and momentum spread (1) in deg. of 1.3 GHz caused by the beam space charge effect.

For the maximum values of Djq, dq from Fig.5 (dq = 0.6%, Djq = 0.16°) and using the algorithm of calculation for the monitor resolution (Dj) from [10] we will get the dependence of Dj vs. the electron phase at the gap entrance (gap with length and rf-voltage of 3 mm and 10 kV, respectively) shown in Fig.6.

j0(deg)

Fig.6. Monitor resolution vs. the electron input phase in deg. of 1.3 GHz.

One can see that in the worse case the monitor resolution is reached of about 0.2°...0.25° of 1.3 GHz within several degrees j0. With installation the target near the beam current maximum the resolution will be in 10 times less. Moreover, estimations have shown that account of the induced charges on the target can improve the resolution significantly. It should be noted that one of the advantages of this technique is possibility to calibrate the monitor using thermoelectrons from the target heated by a current (more in detail of it in [13]).

Streak camera with 0.1 ps temporal resolution

To minimize in 50 times the longitudinal chromatic aberration in an accelerating gap of a streak camera [7] (photocathod - mesh distance) caused by initial electron velocity spread it is proposed instead of a plane - parallel geometry of this unit to use the geometry of the above mentioned one (see Fig.1.b). It will correspond the transition from the right to left side of the curves plotted in Fig.3. Figure 7 makes clear this proposal [14].

Fig.7. Scheme of primary converter for a streak camera with 0.1 ps temporal resolution.

Light is focused by an optic system (1) on a very narrow (about several mm) and thin photocathod (3) being under accelerating voltage of, for example, - 8 kV and placing from the entrance wall of the rf-resonator gap (with longitudinal modulation of the electrons and locked in phase with the beam bunches) of about 1 mm. For reaching high time resolution the transverse rf-modulation is not very convenient due to too much long of fringing rf-field and rf-field aberration. Holder (2) of the cathode (3) is taken very thin, of about 0.1 mm or less, from a free transit light materials to minimize the light dispersion effect. Temporal resolution for proposed device will be mainly defined already only by dispersion effects in windows of the camera, from linac, in Cherenkov radiator and light optics.

There is some more way for improving the time resolution. Time spread of the electrons through the accelerating gap is inverse proportional to root from an initial energy spread of the electrons, i.e. the electrons will have the same time of flight spread in the gap both for the energies from 0 to 1 eV and from 1 to 4 eV. Hence, with monochromotizing of the light at more high frequency one can increase the resolution but this way is not effective in comparison with the proposed one.

It should be noted that the known formula (see 5 in [6]) for estimation of the transit time spread in the gap is not valid for the values about several ps and less.

Transverse beam profile measurement with 5 nm resolution

There is some more advantage of this secondary electron technique: with help the monitor one can measure a transverse beam profile with spatial resolution of 5 nm [14]. In the case (see Fig.1) the resonator is not switched on, instead of the multichannel collector it is permitted to use a single channel one. High spatial resolution is defined by the small magnitude of projection (Dz) of the wire surface, which is visible from the collimator slit Dx0, on the z axis. At the angle of view of 0.1 rad. the projection will be 1.2410-3R0, i.e. at R0 = 4 mm it will be Dz = 5 nm. The thickness of the region in which escaping secondary electrons are produced is about 3 nm [11]. Composition of these two distribution gives FWHM of about 5 nm, i.e. 200 points per 1 mm of a beam.

Plans

We have 6D problem to solve precisely the beam space charge effect in the monitor. The code for this is created now, and we expect to decrease the effect in 10...100 times using additional specific means. In the case we will have to increase the h-distance up to 30 mm.

Acknowledgments

Authors thank A.N.Skrinsky for the encouragement and his interest appeared to this work. A.Tron would like also to thank S.Tazzari and F.Tazzioli for their hospitality during his stay at INFN and express them his sincere gratefulness for returning him to accomplish solution of the problem dealing with the short electron bunch length measurements. Authors are grateful to V.Vaitonis for helping them in preparing the paper.

This work is supported by the Russian Fund for Fundamental Researches under grant No.96-02-18364.

References

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[13] A.M.Tron et.al., "Bunch Phase Distribution Detector for the ISTRA Ion Linac Beam", this Conf.

[14] Tron's proposal