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A HIGH --POSITRON COLLIDING BEAM SYSTEM*

C. Pellegrini, LNF, Frascati; J. Rees, B. Richter, and M. Schwartz, SLAC, Stanford; D. Mahlt and A. Sessler, LBL, Berkeley (Presented by J. Rees)

Abstract the electron ring so that it fits into the same housing re­ sults in an e-p c. m. energy of 65 GeV which is equiva­ A system of two intersecting storage rings of gross lent to 2100 GeV striking stationary . 1 radius 260 m, one for protons and the other for electrons The desi~ luminosity is set at about 1032 cm-2 sec- and positrons, is described. The maximum energy of the for both e+ -e- and e-p collisions based on achieving a stored proton beam is 70 GeV, that of the electron and satisfactory counting rate in some of the more interest­ positron beams 15 GeV; so the center-of-mass ing experiments which can be done with the facility, and are 65 GeV for e-p collisions and 30 GeV for e+ - e- col­ allowing an experimental program of extraordinary lisions. The performance of the system is determined by breadth. the RF power available for the electron and positron beams and by the incoherent beam-bea!lllimit on trans­ This paper describes SOme of the physics which can verse beam density. With an available RF power for the be done with this double-ring system and presents the beams of 2.7 MW, the system yields design luminosities results of our efforts to design the rings. The experi­ in the vicinity of 1032 cm-2 sec-1 in both modes of oper­ ments described below represent only a small fraction of ation. Some important physics experiments and their the physics which can be done with the rings. The topics yields are discussed. discussed were chosen because they are of particular interest now, and they give some idea of the scope of the 1. Introduction possible experimental program. The resulting ring pa­ rameters show that the luminosity specified can be Experiments using the beams from electron and pro­ reached with conventional magnet, RF and injection tech­ ton accelerators have been the driving force in the pursuit niques. We have not attempted to optimize the design for of knowledge in elementary physics. Looking minimum cost, although we think the parameters are back over the last twenty years we see that what we know reasonable. of particle structure comes principally (but not exclu­ 1.1 Physics with 65 GeV (c.m.) Proton-Electron sively) from experiments done at the electron machines, Collisions while our knowledge of particle spectroscopy comes prin­ cipally (but not exclusively) from experiments at proton 1.1.1 Inelastic electron scattering. Inelastic elec­ machines, and our knowledge of particle dynamics comes tron scattering experiments have generated a great deal from experiments at both kinds of machines. The conven­ of interest in the past few years. Recent experiments at tional electron and proton machines - and now the SLAC have revealed a large inelastic cross section, electron-positron and proton-proton colliding beam ma­ giving support to the notion of a grainy substructure in the chines - exist in a kind of symbiotic relationship which proton. With the electron-proton colliding beams, stud­ allows complementary experiments, and is crucial to the ies of the reaction e+p-e+ can be extended to momentum vitality of high energy physics. The maximum center-of­ transfers and inelasticities far beyond anything available' mass (c. m.) energies of the generation of electron stor­ from other machines. age rings now nearing completion lie in the vicinity of 6 GeV. This energy range matches the c.m. energy range It is customary to describe the inelastic scattering of the present generation of conventional accelerators in terms of electrons incident on stationary protons. In (BNL, CERN, SLAC) which lies around 7 GeV. However, these terms, the e-p ring gives an equivalent electron with the advent of the NAL proton soon to laboratory energy of about 2100 GeV. The kinematic pa­ operate with a c. m. energy of 20 to 30 GeV (200 to 500 rameters of interest are q2, the square of the invariant GeV proton beams), and with the CERN ISR operating at four-momentum transferred by the electron and v, the c.m. energies of up to 56 GeV, the proton machines have energy loss of the electron in the system where the tar­ now far outstripped both the electron-positron storage get prot~n is at rest. The maximum value of q2 is 4000 rings and the conventional electron accelerators. (GeVIc) and the maximum value of v is 2100 GeV. This can be compared to a proposed IJ.-p inelastic scattering We have been studying the feasibility of greatly in­ experiment at NAL, which gives a maximum practical q2 creasing the c. m. energy available for electron-positron of 40 (GeVIc)2 and v of 150 GeV with the apparatus colliding beams, and making use of the colliding-beam planned. technique to study electron-proton interaction at c. m. en­ ergies which do not seem accessible with conventional To get an idea of the yields which might be expected accelerators. To this end, we have set our design goals in the e-p ring, we will extrapolate from SLAC energies, in relation to the high energy physics experiments which employing the most generally used theoretical model seem most important, and we have designed a storage (scaling). In bins of dq2/ q2 and dv Iv of ±10%, we find a ring facility to meet those goals. We have chosen a c.m. yield of about 5 eventslday at the maximum momentum energy of 30 GeV for e+ - e- interactions which matches transfer of 4000 (GeV/c)2. For v=1000 GeV in the proton the c. m. energy of NAL at 500 GeV, and represents a rest system, and q2::::1000 (GeV/c)2, we get about 20 large extrapolation in energy from the present generation events per day. These events are quite easy to detect. of e+ -e- rings. Storing the protons in a ring using con­ For example, the case of q2::::1000 (GeVIc)2 and v::::1000 ventional magnets and having the same circumference as GeV gives a final electron of about 20 GeV energy coming out at nearly 900 to the beams, and there are *Work supported by the U.S. Atomic Energy Commission. few background sources which can give such large trans­ verse momenta. tpermanent address: CERN, Geneva. - 154 -

1. 1.2 Photoproduction. Strictly speaking, there is Indeed, there are models which predict even larger than no pure photoproduction in electron-proton collisions. pointiike cross sections at high energies. However, the srecial case of inelastic electron scatter­ 1.2.2 Inclusive hadronic reactions. With 30 GeV ing with q2«me can be looked at as a two-step process ­ first, the of a real , and second, the in­ colliding beams it is possible to study the inclusive reac­ tion e++ e--4 h+ "anything" for large energy and trans­ teraction of this photon to produce . The verse momentum deposited on the one detected h. Weizsacker-Wi1liams approximation gives the equivalent Some of the fundamental questions to be studied in this photon-beam intensity coming from this very low q2 in­ ~hoto­ process are the energy dependence and yields for differ­ elastic scattering, and the effective luminosity for ~,A, production reaction is Q'(k) =0. 07x 1032 (&/k)cm- soo-l, ent hadrons such as 1f, K, N, etc., and the relation of the structure functions to the analogous structure func­ where k is the photon energy. In terms of inci­ tions for deep inelastic scattering from protons. Besides dent on protons at rest, the maximum photon energy is these general studies, specific tests of C invariance, SU3 2100 GeV. invariance, etc. are possible. Estimates all suggest large cross sections and comfortably observable event Counting rates for photoproduction processes range rates for these processes. For example some parton or from very large to very small. For example, the total point-constituent models suggest event rates of from 1 to photon cross section for hadron production is estimated 25 events/hr for a luminosity of 1032/ cm2 sec. to give a yield of 700 (&/k) per second independent of k, while a single p- photoproduction gives a yield of 1.2.3 Two-body final states. Present experiments 70 (&/k), also independent of k. A typical small photo­ on two-body (exclusive) hadron production are not suffi­ production cross section would be that for single- ciently accurate and do not cover a wide enough range in production (yp-4 7l+N). Measurements made up to 20 GeV energy to permit a reliable extrapolation to the storage indicate the energy dependence for this cross section to ring energies considered here. On theoretical grounds, be given by k-2, where k is the photon energy in the however, we would ~xpect hadron form factors falling at proton rest system. In the range of equivalent photon least as fast as 1/E , which would give unobservable energy from 200 GeV to 500 GeV, where photoproduction counting rates at E = 15 GeV with planned luminosities for experiments will complement experiments done with pi pairs, pairs, etc. However, many other two­ hadron beams at NA L, the rate for even this small cross body channels are of great interest and should have large section varies from 15 (&/k) to 2.5 (&/k) events per counting rates. For example, there may exist pointlike hour. Thus, the e-p ring can span most of the spectrum heavy (J.t*) in the mass range 3 $ M * .$15 GeV of photon experiments that have been done with conven­ which are similar to in that they ha~e no strong tional accelerators at lower energy. interactions and pointlike electromagnetic couplings. These will be pair-produced just as ordinary muons are 1. 1. 3 Weak interactions. The basic Fermi inter­ and, for a mass of the IJ. up to 13 GeV, the expected action has a total cross section which rises as the square * counting rate is of order 0.01 per second. The W meson of the c. m. energy until damped by an intermediate discussed previously in connection with the weak interac­ (W) or by some other, as yet, unknown process. tions will be copiously produced electromagnetically if its This dependence has been confirmed to energies as high mass is less than 15 GeV. For a W with magnetic mo­ as several GeV in the c.m. by means of exper­ ment and quadrupole moment of ze~o, we expect a rate of iments at CERN and Brookhaven. If we extrapolate the proportional to m;" and about equal to measured cross section to the 65-GeV c.m. energy of 0.01 per second for m ::::: 14 GeV. the e-p rings, we find it to be about 5 x 10-35 cm2. With w a luminosity of 1032 cm-2 sec-I, this would imply 500 Three other processes of particular interest are p.­ weak interactions per day. It appears quite feasible to pair production, e+e- scattering, and two-quantum anni­ separate these weak interactions from the general back­ hilation. EXisting colliding-beam experiments at Orsay, ground of highly inelastic electromagnetic interactions. Novosibirsk, and Frascati indicate that QED is valid up to a cutoff of 2 or 3 GeV. By increasing the value of the If the (W), which has been hypothesized c.m. energy of the incident pair to 30 GeV, the large to mediate the , exists with a mass less ring will allow precision tests to probe for possible modi­ than 50 - 60 GeV, it should be Kroduced with a cross sec­ fications resulting from cutoffs in the 50 -100 GeV region. tion in the region of 10-36 cm . This would give about 10 production events per day, a very detectable number. 2. Storage Rings 1.2 Physics with 30 GeV (c.m.) e+-e- Colliding Beams 2. 1 General Considerations 1. 2.1 The total hadronic cross section. Experi­ ments in the 1- 2. 5 GeV region in the c. m. have shown The device we consider is shown in Fig. 1. It con­ that both the energy dependence and the magnitude of the sists of two storage rings which intersect each other in total hadronic production cross section are very roughly four places. We consider the case of one bunch in each the same as those for mu-pair production. Such large beam which provides for delivering the maximum possi­ cross sections were not expected at the time of the first ble luminosity at either pair of diametrically opposite attempts to build colliding electron and positron beams, interaction regions. We have only a single tunnel which but this behavior is what we have learned to expect now has the consequence that the protons have, for a reason­ on the basis of constituent models of the hadron such as able design, several times higher maximum energy then those used successfully in explaining deep inelastic the electrons. For the reasons summarized in Section 1, electron-proton scattering. Should the hadronic cross we have chosen 15 GeV for the energy of the stored elec­ section be comparable to the mu-pair cross section at tron beam and hence take 72 GeV for that of the proton very high energies, we can expect hadronic event rates beam, assuming that conventional magnets would be used of order O.Ol/sec at 30 GeV in the c.m. We must, how­ throughout. With superconducting magnets, proton en­ ever, be prepared for major surprises at these energies. ergies up to 150 GeV could be reached. - 155 -

charge density at the interaction region just sufficient to bring the colliding electrons to their incoherent limit, or in other words, the same density as that at which the electron-positron system operates. We find that we can in fact achieve this high proton density despite space­ charge and phase-space density limits. The protons are confined in a single short bunch, as are the electrons, so that all the protons collide with the entire electron swarm and vice versa at each of the two interaction regions. The machine circumference is more than 1000 meters and, in each ring, there is only a single bunch of a few centimeters length.

The luminosity for each interaction region for either kind of collision is

f N1N2 .P =: 4" --p;- , ( 1) int where f is the revolution frequency, Aint is the effective interaction area and N1 and N2 refer to the total numbers of stored in the colliding beams. The revolu­ tion frequencies must of course be the same in both rings. The effective interaction area depends on the heights, PROTON L1NAC widths and lengths of the bunches and the angles. AND BOOSTER 1974Al As argued above, in all cases, the beam limit is the FIG. l--Schematic drawing of the geometric configura­ limit determined by the electron incoherent beam-beam tion of the rings. The electron and positron instability which may be expressed beams cross vertically at an angle of 10 mrad, NN + 2.6.v 'Y and the proton and electron beams cross hori­ ~ e O e (2) zontally at an angle of 10 mrad. A =: A =: e f3; int int In the configuration of Fig. 1 the two rings intersect where r e is the classical electron radiUS, 'Ye is the elec­ at a small angle (10 mrad) in the horizontal plane. At tron energy in rest mass units, f3* is the vertical beta­ the intersection points, the beams in each ring are fo­ tron function at the interaction re~ion in the electron ring cused in both dimensions to a tiny size by low beta opti­ and .6.vO is a parameter which is experimentally - and cal systems. lOne of the rings is designed primarily theoretically - found to be about 0.025 in both e+ - e­ for the storage of protons, haVing variable-frequency and e- - e- storage rings. Now we may write the lumino­ radiofrequency systems and high magnetic field capa­ sities for the two cases as follows: bility. The other ring is designed to store electrons, having a fixed-frequency RF system and smaller mag­ O e f (.6.V 'Y ) [ ] (3) nets. For electron-positron collisions, both beams are .P =: '2 r e f3; Nee or Nep , stored in the electron ring and intersect vertically at a small angle (also 10 mrad) . It is possible also to store where Nee is the number of electrons stored in the case electrons in the proton ring in order to effect e-e colli­ of electron-positron collisions and Ne is that in the case sions; and to store protons in the electron ring to study of electron-proton collisions. The lU~inosity in either p-p collisions. However, in the present study, we ig­ case depends on the parameters of the electron ring nore these possibilities. alone, providing Eq. (2) can be satisfied for both rings.

The fundamental limitations on the e+ - e- colliding­ The number of electrons stored is limited by RF beam performance of electron rings in the energy re­ power considerations. Let Pt> be the total RF power gime under consideration are imposed by the power available to be supplied to the beam or beams in the elec­ radiated from the stored beams as synchrotron radiation, tron ring. which must be supplied by the RF accelerating system and absorbed by the -chamber walls; and by the (4) limit on tolerable transverse space-charge density be­ and yond which one beam disrupts the other (the incoherent beam-beam limit). When the two rings function together Nep =: Pb/fU (5) for electron-proton collisions, the performance of the system again depends on the RF power available for the The radiation loss per turn U is electron beam but not on the electron beam density, assuming the beams are adjusted to the same effective size; because the proton beam, having greater trans­ (6) verse mass, is not disrupted by the electron beam. The performance of the electron-proton system also depends where Pe is the bending radius of the electron beam and on the achievable proton transverse space-charge den­ me c2 is the electron rest energy. The factor of two sity at the interaction regions. We have chosen the pa­ appears in the denominator of Eq. (4) because the RF rameters of the proton ring to achieve a transverse power must be divided between the electrons and the - 156 - positrons when both are stored. In terms of ~, Radiofrequency System Radiofrequency 250 MHz 611 pP ) Harmonic Number 1370 P =22 =~ Oeb (7) 2 2 Total Available Power 5.3 MW ep ee 81l' ( r m c 3 13* • e e 'Ye e Total Accelerating Cavity Length 200 m Total Shunt hnpedance 3. 2x109 ohms We proceed first to the design of the electron ring. Performance at 15 GeY (e+ - e- collisions) 2. 2 Electron Ring Number of Stored Particles (each beam) 1.1XI012 For the lattice we assume a simple separated­ Average Circulating Current (each beam) 30mA function structure which ensures an appropriate distri­ Radiation Loss (U) 45 MeY bution of radiation damping rates. We must choose the Peak RF Voltage 90 MV gross radius of the arcs Rn , the bending radius Pe and Power Radiated by Beam 2.5 MW the beam power Pb so as to achieve the desired lumino­ Power Dissipated in Cavities 2.8 MW sity. Energy Spread (2 x rms) 38 MeY Longitudinal Damping Time 1.8 ms The principal question of feasibility is that of the Beam Width (2 x rms) : Typical 1.4 cm radiofrequency system. The radiation loss per turn U Interaction Region 0.06 cm and therefore the peak accelerating voltage required will Crossing Angle (28) 10 mrad be much higher than those of any existing storage ring or Luminosity (2ee> O. 5xl032 cm-2 sec-1 synchrotron. The peak accelerating voltage requirement is set by the need to achieve a quantum lifetime which is 2.3 The Proton Ring long compared to the storage time. The requirement is The proton ring parameters must be chosen to satisfy a function of various parameters determined by the lat­ Eq. (2) which may be written tice design and of the chosen radiofrequency. Higher voltages are required at high frequencies. We will need N _ 2611 'Y p 0 e peak voltages of the order of 100 MV. Presently opera­ (8) ting systems on the highest energy produce i h*(w*2 +!*2 (2)l!2 - r e 13; peak voltages of the order of 10 MY using copper cavities with total lengths of the order of 10 meters and with in­ in terms of the proton beam parameters, h*, w* and!* stantaneous power inputs of the order of several hundreds which are twice the rms height, width and length respec­ of kilowatts. Thus, we can employ a conventional RF tively, and 0 which is half the crossing angle. The system. . crossing angle is determined by the requirement that the proton and electron beams be separable at the ends of the In selecting the radiofrequency we make a compro­ interaction regions which sets a minimum on O. Since, mise. The shunt impedance per unit length increases for given 0, it is clear that w* can be allowed to be as with frequency, but the peak voltage also increases. For large as !*O before it seriously cuts into the density, and example, the voltage required at a radiofreq1.lency of since, for a variety of reasons, it is desirable to make w* 300 MHz is twice the radiation loss. A reasonable com­ as large as practical, we choose w* =!*O. promise is 250 MHz. The most important constraint on the choice of beam As explained in Section 1, physics requirements parameters is an upper limit on the six-dimensional dictate a design luminosity in the range of 1032 cm-2 phase-space density of the protons u: Under ideal condi­ sec-I. We take this as the luminosity for the electron­ tions, U is preserved from the ion source to the final col­ proton system and so adopt Pee=0.5x 1032 cm-2 sec-I. liding beam condition, but in practice it is reduced by (The total luminosity, summed over all interaction re­ various mishandlings of beams and space-charge blowups. 32 gions, is 10 cm-2 sec-I.) We choose Rn =200 m and four 100-meter-long straight sections in view of the re­ We define normalized emittances by quirement for long RF accelerating structures. The (9) parameters of the electron ring are summarized in EL == 6({Yy)f!* Table 1. '"EH == 1l'({Yy)f w* 2'14 13; (10) Table 1: Electron Ring Parameters E = 1l'({Yy) h *2/4 ,8* (11) Maximum Beam Energy 15 GeY Y f p Lattice where .13~ is the proton lattice function at the crossing Gross Radius of Circular Arcs (Rn) 200 m point (taken the same for horizontal and vertical), 13 and Length of Interaction Regions 100 m 'Yare proton relativistic factors and the subscript f refers Gross Radius (R) 260 m to the final (colliding) energy. Implicit here is the as­ Beta-function at Interaction Point (13x=13y=13*) 0.05 m sumption that the local dispersion at the interaction region Effective Aspect Ratio of Beam at e is small so that the beam width due to momentum spread Interaction Point 0.5 is negligible. With these definitions, Typical Beta-function in Cells 25.1 m Betatron Wave Number in Arcs 12.5 Np=UELEHEy ' (12) Typical Local Dispersion in Cells 3.2m and we have from Eq. (8) Momentum Compaction Coefficient 0.012 Bending Radius (PJ 100 m '" __ __ 1/2 _ 3/2 */ * Bending Field 5.0 kG UEL(EHEy ) - 2 6.IIO'Ye 13p re'Yf13e as a design restraint. - 157 -

We insert a numerical value of a- deduced by examin­ We now employ the beam parameters, as determined ation of existing machines. We take a-=3x 1015 cm-3, a in the previous sections, to determine the injection energy value equal to that corresponding to 95% of the beam in the into the main ring. We adopt an injection kinetic energy CERN PS just after capture at 50 MeV and six times higher of 1 GeV, which value affords a reasonable - but by no than that presently achieved at 19 GeV under the best con­ means optimized - compromise to the various competing ditions with Q-jump at transition. Note that (J is typically considerations. In computing beam parameters at injec­ 3 times higher in the core of a beam (65% rather than 95% tion we have, guided by experience, assumed a factor of of the particles), so our choice is - perhaps - not too ten degradation of phase den:rity in the main ring. Thus optimistic. we employ a-=30x 1015 cm- for injection considerations.

The RF voltage which is required to make a proton The space-charge limit at injection is closely related bunch of length.£* and energy width ~(f3'y>r is a function of to the choice of the RF system, as the RF-harmonic num­ the RF harmonic number ls:f. The minimum voltage Vf, is ber will determine the initial bunching factor. We choose obtained when kf=27T R/£*, and is given by an RF system that will initially work at a frequency around 1 MHz (ki = 6) and fill one bucket of the six avail­ 7T (211 R) 'YIf 2 2 eVf ="2 'Yf ~(,B'Y~ m c , (14) able. We evaluate the space-charge limit taking the ""1* p 12 bunching factor Bi =(2ki) -1 and find Nsc = 8.5 x 10 which is just adequately larger than Np . We note that, despite where 'YIf is given by the very tight bunching at top energy, the space-charge -2 -2 limit is adequate also at top energy. 'YIf = l'Yf - YT 1 ' The primary beam manipulation which is reqUired in with2'YT the transition energy of the proton ring (in units of the main ring, other than acceleration from the injection mpc ). kinetic energy of 1 GeV to top energy of 72 GeV, is a terrific longitudinal beam compression from a bunch For the proton ring we take a filling factor of 6 in o. length of 2. 7x 104 cm to one of 24 em. Basically the the bending sections and a peak field of 20 kG, and hence method to be employed is to use the initial RF system, we obtain 'Yf = 72. For f3p we adopt 15 cm in both trans­ operating on harmonic k = 6, to bunch the beam both by verse dimensions on the assumption that the first quadru­ i accelerating it (adiabatic damping) and by subjecting it to poles at the ends of the crossing region will be employed a much larger voltage than is employed when the beam is to make the very low f3~. We adopt a rather strong focus­ first captured. The first system is then turned off non­ ing structure so that '7f is small; namely we take 'YT=20, adiabatically and a second system operating on a much and an average f3, = 13 meters. We take the RF volt­ higher harmonic k2 (which has been chosen just to tightly age, eVf' to be 10 MeV since, in a practical design, the fit the bunch) is turned on at a low voltage and raised to actual voltage reqUired to obtain a short bunch is approxi­ a high voltage thus further compressing the bunch. The mately four times this value, and hence the actual eVf is process is repeated as often as necessary (two or three similar to that in the electron ring. The resulting param­ times), finally employing a system which requires eters of the proton ring are given in Table 2. approximately 40 MV per turn. Only the final system Table 2: Proton Ring Parameters has to work at this very high voltage level. Space-charge effects at transition also require a large RF voltage Maximum Beam Energy 72 GeV (30 MY). Lattice Gross Radius (R) 260 m Reference Beta-function at Interaction Point (f3p> 0.15 m Typical Beta-function in Cells 13 m 1. See the follOWing for discussions of the concepts Transition Gamma (')IT) 20 employed in Section 2: M. Sands, "The Physics of 120 m Bending Radius (Pp) Electron Storage Rings, an Introduction, " in Physics Bending Field 20 kG with Intersecting Storage Rings, edited by Radiofrequency System (final system) B. Touschek (Academic Press, New York and Lon­ Radiofrequency 250 MHz don, 1971). (This work is also available as Stanford Harmonic Number (kf) 1260 Linear Accelerator Center Report No. SLAC-121, Peak RF Voltage 40 MV November, 1970.) H. Bruck, Accelerateurs Performance at 72 GeV Circulaires de Particules (Presses Universitaires de France, Paris, 1966). Number of Stored Protons (NP> 7.5x1012 Beam Width (2xrms) (w*) 0.12 em Beam Height (2 x rms) (h *) 0.06 em Bunch Length (2 x rms) (t*) 23 em Momentum Spread [~(/3y>rJ 0.17 Injection Parameters Injection Kinetic Energy 1 GeV Radiofrequency 1 MHz Harmonic Number 6 Beam Width (2xrms) 4.8 em Beam Height (2x rms) 2.2 em Bunch Length (2x rms) 270 m Momentum Spread [~(fYy)J 1. Ox 10-4 - 158 -

DISCUSSION

F. MILLS: Do you have designs for the 5 cm and R. SANTANGELO: If I understand correctly~ the 15 cm S-functions ? machine you have discussed is not able to study electron-electron interactions~ but only electron­ J. REES: No. positron interactions. What are the main reasons for such a choice? In fact~ a trivial comparison F. MILLS How much free space is in the straight between p-p storage rings and perhaps also a study sections ? of photon-photon interactions~ should point out also the interest of an electron-electron machine at J. REES: The r.f. system occupies half the total comparable energy. free space in the long straight sections in the electron ring. The remainder can be used for op­ J. REES: You are correct to suggest that there are tical elements and deteciors. good reasons for studying the e-e- collisions~ and the double-ring system can certainly be built to accomplish it by equipping one ring to store either B.W. MONTAGUE: Have you attempted to equalise the electrons or protons. Indeed both rings could be longitudinal and transverse emittances in the proton built that way to achieve pp collisions too. In our ring to avoid dilution of phase-space density due to initial studies~ however~ we have limited our con­ coupling ? siderations arbitrarily to the performance of the e+e- and ep systems. A.M. SESSLER We have not in our initial studies.