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REVIEW 3 major objections 5 minor 4 references

Further searches of the Higgs scalar sector at the ESS

T0 review · 3 major / 5 minor · reviewed 2026-08-14 · deepseek-v4-flash

Pith's one-line read The paper argues that a muon collider built as an extension of the Lund spallation source could deliver about 12,000 clean Higgs events per year at the Higgs mass, provided ionization cooling reaches its target compression.

desk verdict Rubbia's ESS muon collider paper has a strong physics case and an honest limitation statement, but the 12,000 events/year headline rests on an unproven cooling extrapolation that should be the central referee issue. read the letter →

arxiv 1908.05664 v3 pith:GC4KI5I4 submitted 2019-08-14 physics.acc-ph hep-ex

classification physics.acc-phhep-ex
keywords muoncolliderHiggsfactoryionizationcoolings-channelproductionEuropeanSpallationSource6Dphase-spaceRFOFOringluminosity
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The paper argues that the European Spallation Source, already being built for neutron science, could be extended into a muon collider that studies the Higgs boson far more cleanly than hadron colliders can. Because the Higgs couples to leptons in proportion to the square of their mass, colliding muon pairs at $\sqrt{s}=125.5$ GeV puts the Higgs on resonance, with a sizeable signal and small backgrounds. The author lays out a full chain—proton accumulation, pion production, muon capture, ionization cooling, recirculating acceleration, and a compact 60-m-radius collider ring—that would yield about 12,000 Higgs events per year at each interaction point. The load-bearing step is six-dimensional ionization cooling: the scheme needs a phase-space compression merit factor near 15,000, far beyond the largest simulated cooling ring result of 162 after 16 turns. The paper therefore pairs the collider proposal with a staged, inexpensive Initial Cooling Experiment intended to demonstrate that compression before committing to the full machine.

What carries the argument

The machinery is ionization cooling. Muons pass through liquid-hydrogen wedges, losing momentum in all three dimensions through ionization; radio-frequency cavities restore only the longitudinal momentum, so the transverse emittance shrinks until multiple Coulomb scattering balances the cooling at an equilibrium emittance. The paper's rate estimate is carried by the merit factor $M=(\text{initial 6D emittance})/(\text{final 6D emittance})\times\text{transmission}$, which must be about 15,000, and by the luminosity formula $L=fN_+N_-/(4\pi\varepsilon_{\text{rms}}\beta^*)$, with $\beta^*=5$ cm at the two collision points. Cooling takes place in a sequence of rings, notably the RFOFO ring of alternating tilted solenoids whose simulation gives a merit factor of 162 after 16 turns; the paper assumes that doubling the number of turns plus a linear pre-cooling stage reaches equilibrium. A recirculating linear accelerator with nine passes carries the muons from 2.5 GeV to 62.5 GeV, and the final collider ring has a 60 m radius at about 7 T.

What would settle it

Run the proposed Initial Cooling Experiment with an RFOFO-like ring at 250 MeV/c for 32 turns and measure the six-dimensional merit factor; if it falls substantially short of about 15,000—for instance if the equilibrium transverse emittance stays above the $0.4\pi$ mm rad target at acceptable transmission—then the luminosity and 12,000-events-per-year figure collapse. A second decisive test is a measurement of the achievable beam-energy spread at 62.5 GeV: if the relative spread cannot reach $R=0.003\%$, the effective Higgs cross section drops by roughly a factor of two to four, and the physics reach is correspondingly reduced.

Watch

Extended reading notes

Core claim

The central claim is that a muon collider built as an extension of the ESS proton linac can operate as a Higgs factory in the s-channel: with about $2.9\times10^{12}$ positive and $1.9\times10^{12}$ negative muons per bunch after cooling and acceleration to 62.5 GeV, two interaction points reach $L = 4.0\times10^{31}\,\text{cm}^{-2}\text{s}^{-1}$ and accumulate roughly 12,000 Higgs events per year at $\sqrt{s}=125.5$ GeV. This event rate, together with the very favourable signal-to-background ratio of the $H\to WW^*$ channel (about 100:1) and the near-background-free environment, would allow direct measurement of the Higgs total width and the muon Yukawa coupling, and high-precision study of the main decay modes. The author also describes a higher-energy option at $\sqrt{s}\approx700$ GeV for Higgs-strahlung, vector-boson fusion, and double-Higgs processes, and notes that parametric-resonance ionization cooling, if it works, could raise the luminosity or cut the required proton intensity by about an order of magnitude.

Load-bearing premise

The load-bearing premise is that ionization cooling can squeeze the muon beams by a factor of about 15,000 in six-dimensional phase space, even though the best simulated cooling ring achieves only 162 after 16 turns and the full end-to-end system has not been simulated.

Editorial extensions

If this is right

  • If the cooling target is met, the ESS muon collider would deliver roughly 12,000 Higgs events per year at each interaction point in an essentially background-free environment, enabling a direct measurement of the Higgs width and the muon Yukawa coupling.
  • The same compact footprint—a 60 m collider radius at 7 T plus the existing spallation-source linac—would allow a staged program in which the Initial Cooling Experiment de-risks the full machine at modest cost.
  • A successful measurement of the Higgs mass via the $(g-2)$ precession of polarized muons to about 100 keV would make the resonance scan and line-shape measurement far sharper than what hadron colliders can provide.
  • If parametric-resonance ionization cooling succeeds at the required intensity, the luminosity could increase or the required proton rate could drop by roughly an order of magnitude.
  • The higher-energy option at $\sqrt{s}\approx700$ GeV would extend the programme to Higgs-strahlung, vector-boson fusion, and double-Higgs production with a ring radius of about 220 m, still far smaller than proposed electron-positron circular colliders.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • A reader should treat the Initial Cooling Experiment not as a small demo but as the decisive test of the whole proposal, since every downstream number scales linearly with the achieved merit factor.
  • The energy-spread requirement of $R=0.003\%$ is as important as luminosity: if the muon beam energy cannot be controlled to about 100 keV via the $(g-2)$ frequency measurement, the effective s-channel Higgs cross section drops from roughly 22 pb toward 10 pb, eroding the event-rate advantage.
  • The decay-electron shower power of about 1.6 kW/m from muon decays will dominate machine and detector shielding design; even with perfect cooling, managing this background is an engineering constraint the paper acknowledges but does not fully solve.
  • If the cooling chain works at the spallation source, the same muon-production and cooling infrastructure could be shared with a neutrino programme, so a successful cooling demonstration would strengthen both projects together.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

3 major / 5 minor

Summary. This manuscript (arXiv:1908.05664) proposes a staged extension of the European Spallation Source (ESS) into a muon-collider complex called ESSmuSB, aimed at studying the Higgs scalar sector. The proton-beam section (Sec. 8) envisions operating the ESS linac at doubled duty cycle, accumulating H- ions via charge-exchange injection, and compressing 2.5 x 10^14 protons into ~2 ns bunches at 56 Hz. The muon-production section (Sec. 9) uses a 20 T solenoid field for pion capture from a mercury target, followed by drift, bunching, and phase rotation to ~250 MeV/c. Section 10 describes a cooling chain (linear transverse pre-cooling, 6D cooling in RFOFO-type rings, and high-field solenoidal cooling) targeting normalized emittances of 0.4 mm mrad (transverse) and 1.0 mm mrad (longitudinal), i.e., a 6D compression factor of 75,000 with merit ~15,000. Section 11 proposes recirculating-linac acceleration to 62.5 GeV, and Sec. 12 presents the collider: a 350 m ring with beta* = 5 cm, two interaction points, L = 4.0 x 10^31 cm^-2 s^-1 per IP (averaged over the 56 Hz store cycle), and ~12,000 s-channel Higgs events per year at sqrt(s) = 125.5 GeV with beam energy resolution R = 0.003%. A ~700 GeV option and a parametric-ionization-cooling (PIC) upgrade are sketched, and Sec. 14 proposes a modest Initial Cooling Experiment to validate muon cooling before full-scale construction.

Significance. If the assumed cooling performance were achieved, the physics case would be compelling: s-channel mu+ mu- -> H production at the tens-of-pb level with very small backgrounds would permit a direct measurement of the Higgs total width and the muon Yukawa coupling, complementing the LHC and e+e- programs. The luminosity arithmetic is transparent and reproducible from Table 3: f = 29,970/s, N = 2.41 x 10^12, epsilon_rms = 0.62 x 10^-4 cm rad, beta* = 5 cm give L ~ 4 x 10^31 cm^-2 s^-1, and the 12,000 events/yr follows from L x 3 x 10^-35 cm^2 x 10^7 s. The manuscript deserves credit for proposing a concrete, falsifiable experimental milestone (the RFOFO-based Initial Cooling Experiment of Sec. 14), for explicitly flagging its own open problems (the missing integrated cooling design in Sec. 10; foil/laser stripping R&D in Sec. 8; the 'bold extrapolations' for PIC in Sec. 13), and for a balanced historical account of the US muon-cooling literature.

major comments (3)
  1. [Section 10 (pp. 31-38, Fig. 28, Eq. (3))] The central quantitative claims rest on a 6D phase-space compression of 75,000 (from epsilon_perp = 20 mm mrad and epsilon_L = 30 mm mrad to 0.4 and 1.0 mm mrad, i.e., merit ~15,000 after a factor-5 transmission loss), yet the only simulated cooling point cited is the RFOFO ring with 6D merit 162 after 16 turns (Fig. 28; Ref. [48]). The bridging sentence — that 'doubling the number of turns of the RFOFO cooling ring will ensure — with the addition of the required phase of linear pre-cooling — the required compression to attain equilibrium of emittances' (p. 38) — does not close the gap. Stacking the evidence as generously as possible: the linear pre-cooler takes epsilon_perp from 20 to 3 mm mrad per plane (p. 32), contributing at most 6.7^2 ~ 45 to the 6D volume reduction (and the text states this stage grows the longitudinal emittance, so its 6D contribution is less); combining with the RFOFO merit of 162 gives ~7 x 10^3, an order of magnitude below 7.5 x 10^4. Doubling the ring turns cannot supply a factor ~10: the same paragraph states that after 16 turns the emittances were already 'at equilibrium', and at equilibrium the cooling decrement vanishes (Eq. (3)), so extra turns add only decay losses (at 250 MeV/c the ~5.6 micro-s lifetime is ~47 ring turns, so 16 extra turns cost ~25-30% intensity). Since N_mu after cooling enters L linearly, this issue is load-bearing, and the paper itself acknowledges (p. 33) that 'an integrated design including the full complexity of the beam transports, reacceleration and bunching, and including nonlinear beam dynamics coupled with the ionization interactions, are still missing.' The manuscript should either present a simulation-based path to the required merit factor or re-state L = 4 x 10^31 cm^-2 s^-1 and the 12,000 events/yr as conditional targets with the scaling in merit factor made explicit.
  2. [Table 2] Table 2 contains internal inconsistencies that must be corrected before it can serve as the muon budget. Applying the stated stage survival factors to the negative-muon column yields 1.34 x 10^13 mu-/pulse after linear transverse pre-cooling (0.7 x 1.91 x 10^13) and 8.02 x 10^12 mu-/pulse after RFOFO cooling before merging, whereas the table prints 1.34 x 10^12 and 8.02 x 10^13, respectively; the subsequent rows (6.42 x 10^12, 3.85 x 10^12, 2.70 x 10^12, 1.89 x 10^12) agree only with the corrected values, confirming order-of-magnitude transcription errors. In addition, the quoted 'Total survival factor of the process 0.07' equals neither the product of the tabulated stage factors (0.7 x 0.6 x 0.8 x 0.6 x 0.7 x 0.7 = 0.099) nor that product times the 0.8 front-end survival stated in Sec. 9 (~0.079); the basis for 0.07 should be stated explicitly.
  3. [Section 9 (p. 27)] The pion yields that seed the entire muon budget — 6.72 x 10^13 and 4.15 x 10^13 pi+/pi- per pulse at all angles, and 2.97 x 10^13 and 1.91 x 10^13 forward with 50-600 MeV/c — are attributed to 'a GEANT4 simulation at the ESS', but the simulation geometry, physics list, scoring, statistical uncertainty, and any benchmark against published hadroproduction data are not shown, and no reference is supplied. Because the final muon intensities, the luminosity, and the event rate all scale linearly with these yields, the paper should either present the yield distribution with its input assumptions or explicitly label these numbers as assumptions and quantify the sensitivity of L and the event rate to a plausible range of pion yields.
minor comments (5)
  1. [Table 3 vs. Section 4] Table 3 converts luminosity to event rate with a 'Nominal Higgs cross section' of 3.0 x 10^-35 cm^2 (30 pb), while Section 4 and the concluding remarks quote an effective s-channel cross section of 22 pb with ISR and BES effects included at R = 0.003%; at 22 pb the headline would be ~8,800 events/yr rather than 12,000. The table, the text, and the event count should be harmonized.
  2. [Section 12 (Table 3)] The luminosity formula L = f N+ N- / (4 pi epsilon_rms beta*) contains no hourglass factor, yet the quoted longitudinal invariant emittance (1.9 mm mrad, once its convention is fixed) and the required R = 3 x 10^-5 imply a collision sigma_z of order 10 cm, comparable to or larger than beta* = 5 cm; the paper should state the collision-bunch longitudinal parameters, explain how the ~30 cm rms bunch at 250 MeV/c (which grows adiabatically with sqrt(gamma) during acceleration) is re-bunched, and include the resulting hourglass correction.
  3. [Section 14 (pp. 50-51)] The ring period is quoted as 162.51 ns and also as being 'accurately adjusted to 40 RF cycles' at 234.8 MHz, but 40 cycles at 234.8 MHz is 170.4 ns; the two statements disagree by about 5%.
  4. [Throughout] The text contains several garbled or duplicated passages that impede reading: the abstract truncates and repeats sentences ('...only capable to perform Ho related measurements...', 'should be investigated Ho has a spin zero'), 'Louvillian' appears for 'Liouvillian' (Secs. 9, 10, 12), a stray bracket appears in 'RFOFO ring of 45 m circumference]' (Sec. 14), and 'conference of about 45 meters' should read 'circumference'. The reference list also needs cleanup: [36] is used twice (JUNO and RENO-50), [56] contains a stray '[14]', and [63]-[64] are not cited in the text.
  5. [Section 12] The origin of the factor 54 in f = 54 x 555 = 29,970 s^-1 (as opposed to the 56 proton-collision rate per second) is not explained; the effective-turns bookkeeping (555 ~ half the turns in one muon lifetime in the 350 m ring) is otherwise clear.

Circularity Check

0 steps flagged · score 0.0 of 10

No circularity found: the luminosity and event-rate claims rest on stated assumptions and externally simulated cooling parameters, not on fitting the target result back into the inputs.

full rationale

The derivation chain from proton pulses to Higgs event rate is not circular. The luminosity is computed with the standard formula L = f N+ N-/(4π ε_rms β*) using N± = 2.41e12, ε_rms = 0.673e-4 π cm rad, and β* = 5 cm as stated inputs; none of these is fitted to the quoted 12,000 events/yr. The muon intensities in Table 2 are obtained by multiplying the GEANT4 pion production rate by an explicit chain of transmission efficiencies, and the paper does not invert the event rate to recover any of those efficiencies. The final equilibrium emittances (ε⊥ = 0.4π mm rad, εL = 1.0π mm rad) are imported from the COOL 2007/RFOFO simulations (Refs. 13, 48) and used as input assumptions, not derived from the luminosity target. The most vulnerable step—asserting that doubling the RFOFO turns gives the required merit factor—is an extrapolation from Ref. 48's merit figure of 162 and is explicitly acknowledged as not yet integrated: the paper states that 'an integrated design including the full complexity of the beam transports, reacceleration and bunching, and including nonlinear beam dynamics coupled with the ionization interactions, are still missing.' A weak or unsupported extrapolation is a correctness risk, not a circular reduction. Self-citations appear only in historical and background contexts (e.g., Ref. 12) and are not load-bearing for the luminosity or event-rate claims. No equation in the paper defines its prediction in terms of its conclusion, and no fitted parameter is renamed as a prediction. The design is therefore self-contained in the circularity sense, with the cooling feasibility question left honestly open to the proposed Initial Cooling Experiment.

Assumptions & free parameters 5 free parameters · 5 assumptions · 0 invented entities

The quoted luminosity and event rate depend directly on hand-assigned stage survival factors and assumed cooling equilibrium emittances. The GEANT4-based pion yields are not shown. No free parameter is fit to measured data; rather, several values are chosen to make the final event rate reach the stated 12,000 per year.

free parameters (5)
  • Stage survival factors (Table 2) = 0.7, 0.6, 0.8, 0.6, 0.7, 0.7
    These chosen transmission efficiencies determine the final muon counts (2.93e12 and 1.89e12) and therefore the luminosity; they are not derived from a shown simulation.
  • Cooling merit factor = ~15,000
    The required 6D compression factor of 75,000 with transmission 1/5 is assumed by extrapolating the RFOFO ring merit factor of 162 after 16 turns to 'doubling the number of turns' (Section 10).
  • Equilibrium normalized emittances = 0.4 pi mm rad transverse, 1.0 pi mm rad longitudinal
    Taken from prior hydrogen cooling simulations (cited [48], [49]); they set the collider luminosity.
  • Proton bunching factor b = 1/60
    Assumed to compute the Laslett tune shift and the 1.98 ns r.m.s. compressed bunch length (Section 8).
  • Beam energy resolution R = 0.003%
    Imposed to resolve the 4.2 MeV Higgs width; this drives the extremely low momentum spread required at the collider.
assumptions (5)
  • domain assumption The observed 125.5 GeV Higgs boson is Standard Model-like, with total width about 4.2 MeV and standard branching fractions.
    Used throughout Sections 2 and 4 to compute cross sections, event rates, and required energy resolution; based on LHC measurements cited in [1], [2].
  • domain assumption The ESS linac can be upgraded to 28 Hz, operate with H- ions, and feed accumulator and compressor rings with charge-exchange injection.
    Required for the 56 Hz proton delivery in Section 8; not part of the approved ESS baseline, and the paper states foil and laser stripping both need further development.
  • domain assumption Ionization cooling can reach normalized equilibrium emittances of 0.4 pi mm rad transverse and 1.0 pi mm rad longitudinal, with an overall merit factor near 15,000.
    Central to muon intensity; the paper says cooling has not been experimentally demonstrated and an integrated design is still missing (Section 10).
  • domain assumption The pion and muon yields are those from an unshown GEANT4 simulation of a 30 cm mercury target in a 20 T solenoid.
    Section 9 states the simulation was used but provides no geometry, physics list, or comparison with data, so the yields are taken as input.
  • domain assumption Pressurized hydrogen-filled RF cavities can sustain gradients up to 330 MV/m at 50 atm and 77 K.
    Used for the high-gradient cooling channel in Sections 10 and 14, based on cited Freemire and Chung work; not demonstrated at the scale required.

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Pith. "Pith review of Further searches of the Higgs scalar sector at the ESS." pith.science (2026). https://pith.science/paper/GC4KI5I4

@misc{pith2026190805664,
  author       = {Pith},
  title        = {Pith review of: Further searches of the Higgs scalar sector at the ESS},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/GC4KI5I4}},
  note         = {Machine review of arXiv:1908.05664}
}
read the original abstract

Recent decades have witnessed remarkable confirmations of the Standard Model (SM) describing the Electro-Weak and Strong Interactions. The Higgs boson was observed at CERN-LHC at 7-8 TeV and 13 TeV. The HL-LHC, a major luminosity upgrade has been recently approved. The HL-LHC may be already an early "Higgs factory", however only capable to perform Ho related measurements with rather large uncertainties because of persisting backgrounds and uncertainties. New projects using leptons rather than hadrons should be investigated Ho has a spin zero and its coupling is proportional to the square of the lepton mass, greatly enhancing the production from pairs of muons. A mu+mu- Collider may operate at a much higher magnetic field respect to the e+e- Collider and it has a smaller radius, easily fitting within one existing European site. However muons are unstable particles: they must be produced in sufficient amounts from pions of a proton beam, cooled and quickly accelerated to the required energies. The scenario is here primarily concentrated to further developments of the European Spallation Source (ESS) under construction in the Lund site as the most intense future source of spallation neutrons. As a initial part of the program, muon cooling should be experimentally demonstrated with the much cheaper and simpler Initial Cooling Experiment.

Figures

Figures reproduced from arXiv: 1908.05664 by the authors.

Figure 2
Figure 2. According to the Standard Model (SM), the width of the Ho is only ≈ 4.2 MeV, compared for instance to the much larger Zo width of 2.5 GeV [PITH_FULL_IMAGE:figures/full_fig_p004_2.png] view at source ↗
Figure 3
Figure 3. Leading Higgs channels as a function of the Higgs mass. The Liouville theorem [54] states that whenever there is a Hamiltonian (i.e. a force derivable from a potential) the six dimensional phase space of the beam (qi, are positions and pi conjugate momenta) is preserved, namely, dV/dt = 0, since the rate of [PITH_FULL_IMAGE:figures/full_fig_p004_3.png] view at source ↗
Figure 4
Figure 4. Main components of a Muon Collider as described in COOL-2007 [13]; Phase (#1) is the phase rotation;(#2) initial cooling; (#3) 201Mhz 6D cool; (#4) 402 Mhz 6D cool; (#5) merge to single bunch; (#6) 201Mhz 6D cool; (#7) 402Mhz 6D cool; (#8) 805 Mhz 6D cool; (#9) transverse cool at 50 Tesla; acceleration and Collider ring. During the subsequent two decades, Neuffer, Palmer, Cline and many others in the US and elsewher… view at source ↗
Figures from the paper (26 more)
Figure 6
Figure 6. Figure 6: Several other new projects based on circular rings of e+e- described for different locations world wide. Several other new projects based on e+e- have also been described for different locations ( [PITH_FULL_IMAGE:figures/full_fig_p008_6.png]
Figure 12
Figure 12. Figure 12: The ESSνSB and the ESSµSB, are dedicated to the neutrino and muon programmes. High intensity bunches from the negative H- source are converted into protons, producing secondary particles (mostly π±). The π decay to μ’s and the μ’s are then captured, bunched, cooled an…
Figure 13
Figure 13. Figure 13: Layout of the ESSνSB project. The repetition rate of the LINAC could be doubled from 14 Hz to 28 Hz with the additional 5 MW protons to new facilities. To this effect, (H-) ions, instead of protons (H+), are accelerated by the LINAC. The (H- ) ions will then be stripp…
Figure 14
Figure 14. Figure 14: In view of the low neutrino energy and the very high intensity of the ESS proton beam, the far more preferable 2nd oscillation maximum has been shown for neutrinos and for various indicative values of the dCP phase. The CERN-SPL [30] design ( [PITH_FULL_IMAGE:figures…
Figure 15
Figure 15. Figure 15: The CERN-SPL design [27] is made of a 160 MeV normal conducting sequence of four accelerating structures of Linac (RFQ, DTL, CCDTL and PIMS) followed by a 2.0 K superconducting Linac producing a H- beam with about 5 GeV kinetic energy. In the full HP-HPL version of th…
Figure 16
Figure 16. Figure 16: The LINAC beam with 5 MWatt pulses is firstly accumulated in a thin stripper. A pair of proton rings subdivide the beam into four pulses extract the proton beam at 56 Hz, i.e. with bunches every 17.8 ms and 2.5 x 1014 p/bunch. In view of its relatively modest energy a…
Figure 17
Figure 17. Figure 17: Foil stripper temperature vs. particle density [22]. To compute the foil temperature, the carbon foil thickness of 300 µg/cm2, an emissivity of 0.7 and a repetition rate of 50 Hz have been chosen. The feasibility of the injection has been studied using the tracking co…
Figure 18
Figure 18. Figure 18: General description of the LASER driven stripping method. Negative hydrogen atoms are stripped into neutral with a high magnetic field, excited with a resonant Laser to (n = 3) and finally stripped into protons again with a high magnetic field. An efficiency of 90% ha…
Figure 19
Figure 19. Figure 19: (a) Momentum distribution vs the RF phase angle of the compressor before and after the bunch rotation of the proton beam and (b) beam rotated to s = 1.98 ns r.m.s. RF phase angles are given in units of three degrees. Bringing the energy to 3.5 GeV and with the same 5 …
Figure 20
Figure 20. Figure 20: Charged pion momentum spectra for 2 GeV and 5 GeV protons on a 30 cm long heavy Z (mercury) target. The production of secondary particles after the target will be performed in several phases to be described in the following paragraphs in more detail: a first phase wit…
Figure 21
Figure 21. Figure 21: Secondary particles of both signs are produced in a axially symmetric horn with a 30 cm target cm long heavy Z (mercury) target immersed in a high field solenoid at a longitudinal Bo = 20 T field. The proton beam is oriented with respect to the target at an angle of 2…
Figure 25
Figure 25. Figure 25: Following Neuffer et al. [46] after the extraction from the solenoid, secondaries of both signs are momentum analysed with a magnetic structure called “HFOFO Snake” or “chicane” ( [PITH_FULL_IMAGE:figures/full_fig_p028_25.png]
Figure 22
Figure 22. Figure 22: The muon distribution with large energy spread and small bunch length stretches to an energy-position correlation in the Drift. The RF-Buncher forms the beam into a string of different energy bunches and the RF-Rotator moves bunches to equal energies, forming a string…
Figure 25
Figure 25. Figure 25: Complete scheme for a muon Collider given in COOL 2007 by the US team [64], but adapted to the case of the ESS. This process is there numbered from, (#1) to (#9). Transverse emittances are 6D cooled in H2 from 10 to 0.4 (π) mm rad and longitudinal emittance from 30 to…
Figure 26
Figure 26. Figure 26: After the extraction from the solenoid, secondaries of both signs may be momentum analysed with a magnetic “HFOFO Snake” or “chicane”, orbit distortion. The muon does not have strong interactions. Its higher mass relative to the electron means that it can pass through…
Figure 27
Figure 27. Figure 27: Alternative ring configurations: Tetra ring (Balbekov), RFOFO ring (Palmer) and Guggenheim ring (Klier) In order to describe in more detail Ionization Cooling, we will look initially at the effects in the transverse plane (perpendicular to the beam trajectory) and the…
Figure 28
Figure 28. Figure 28: Example [48] of a “RFOFO” Cooling Ring (“FOFO” since “both focus” and “R for ‘reverse”). The three emittances and transmission are plotted on a log scale versus distance. Focusing is provided by pairs of solenoids with alternating field directions. All cells are ident…
Figure 29
Figure 29. Figure 29: Schematic drawing of the four-sided ring cooler using dipoles and solenoids in the configuration of Garren et al. [49]. In order to cool the beam, the liquid hydrogen (LH2) wedge coolers will be inserted into a region with low and high dispersion [PITH_FULL_IMAGE:fig…
Figure 30
Figure 30. Figure 30: Schematic drawing of the ring quadrant in the four-sided and achromatic ring cooler [PITH_FULL_IMAGE:figures/full_fig_p040_30.png]
Figure 32
Figure 32. Figure 32: Aa acceleration system is progressively rising the energy of muons to mHo/2 with the help of re-circulating linear accelerators (LRA). For instance with a eight turn arrangement the energy increase of the LRA is 7.8 GeV/pass, corresponding to a length of ≈ 350 m for a…
Figure 33
Figure 33. Figure 33: Lattice structure at crossing point of the 60 m radiua ESS Collider,including local chromaticity corrections with bx = by = b* = 5 cm An important background which has to be carefully analyzed is coming from the ≈ 2 x 1012 muons/bunch of each sign from decays, emittin…
Figure 34
Figure 34. Figure 34: The amount of power due to 1.9 x107 decays per m of electron showering coming from 6 x1012 decays is very large and it must be handled with an appropriate geometry of the locations of the shower stoppers. The angular distribution of the decay electrons and positrons s…
Figure 35
Figure 35. Figure 35: Presently the Higgs mass is known to some 600 MeV., At the muon collider we need to locate MH to ~ 4 MeV. The location of the resonance can be performed initially with a few months running at the relatively modest initial 1.7 x 1031 luminosity. The present uncertainty…
Figure 36
Figure 36. Figure 36: LEFT ordinary oscillations; RIGHT hyperbolic motion induced by perturbations near an (one half integer) resonance of the betatron frequency. PIC dynamics is expected to produce a smaller final transverse beam emittances and may offer the potentials either for a higher…
Figure 37
Figure 37. Figure 37: Schematic description of the PIC cooling. Muons from the front end are entering n the main cooling ring where transverse emittances rreach the cooling equilibrium. After further acceleration to about 1 GeV/c a second larger ring at the PIC configuration near a resonan…
Figure 38
Figure 38. Figure 38: The “RFOFO” ring of 45 m circumference] is made of 12 identical cells with about 3 degrees tilted solenoids of opposite orientations providing focusing and bending. RF cavities may be either under vacuum or pressurized with hydrogen and helium gas up to more than 100 …

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Works this paper leans on

4 extracted references · 3 canonical work pages

  1. [2]

    The first term is the ionization loss and the second term is the multiple scattering

    with b* the value of the betatron function at the crossing point, mµ and bµ the values relative to the muon for the radiation length Xo in cm and dE/dz the ionization loss.in MeV/cm. The first term is the ionization loss and the second term is the multiple scattering. The Bethe Bloch parameters for several materials are shown in Table 1. The cooling proce...

  2. [3]

    dE/dx foil

    The invariant, normalized equilibrium r.m.s. emittance (eV,H) with and the corresponding actual transverse emittance (eV,H /bg) are function of the muon momentum. For liquid H2 and cooling at b*= 10 cm, dεH,Vdz=εH,Vβ2EdEdz+β*13.6 MeV/c()2β2EmµXo2→0εV,H→β*13.6 MeV/c()22βµmµ1XodEdz()ε=σxσθ=sqrtx2θX2−xθX2() 34 eV,H ≤ 370 mm mr at 250 MeV/c. In the case of Li...

  3. [4]

    where the first term is the intrinsic energy loss, the second is the wedge shaped absorber and the third the straggling contribution. Therewhere fA is the fraction of the transport length occupied by the absorber, which has an energy absorption coefficient ; h is the chromatic dispersion at the absorber and d and are the thickness and radial tilt of the a...

  4. [5]

    RFOFO” Cooling Ring. Focusing is provided by pairs of solenoids with alternating field directions (“FOFO

    where Xo is the radiation length, mec2 the electron mass and a the fine structure constant. Reaching the equilibrium conditions, the above indicated straggling contribution is exactly balanced by the first two terms. Since this increases as g2 + 1, cooling at low energies is desired. For 200 MeV/c, 120 MeV, 0.88c, we find 1.2 km and 4.6 MeV/gr cm2. Balanc...

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Reviewed August 14, 2026 · model on record in the stance chip above.