Very Asymmetric Collider for Dark Matter Search below 1 GeV

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Presentation transcript:

Very Asymmetric Collider for Dark Matter Search below 1 GeV B. Wojtsekhowski, V.S. Morozov, and Y.S. Derbenev Jefferson Lab, Newport News, VA 23606 U.S. Cosmic Visions: New Ideas in Dark Matter 23-25 March 2017, University of Maryland, College Park F. Lin

Evidence for Light Dark Matter P. Jean et al., Astron. Astrophys. 445, 579 (2006) 511 keV line in the photon spectrum Photon energy spectrum Location of the source

Direct Observation NASA/SLAC, September 2006 Collision of two large clusters of galaxies

Search for New Particle Search for single-photon events 𝑒 + 𝑒 − →𝛾𝐴′ Seek a narrow peak in the distribution of 𝑀 𝑋 2 =𝑠−2 𝐸 𝛾 ∗ 𝑠 Lowest-order Feynman diagram of 𝑒 + 𝑒 − →𝛾+ 𝐴 ′ Need a low-energy high-luminosity electron-positron collider 𝐴 ′ 𝑠~4 𝐸 + ⋅( 𝐸 − − 𝐸 𝛾 ) Δℒ~ℒ× Δ𝑠 𝑠 𝑚𝑎𝑥 ; 𝑠 𝑚𝑎𝑥 =10 𝐺𝑒𝑉, Δ𝑠 ~100 𝑀𝑒𝑉 ⇒Δℒ~ 10 −4 ℒ

Collider Luminosity Collider luminosity generally drops off with energy Geometric emittances/ beam sizes are larger at lower energies Beams are less rigid and cannot interact strongly at lower energies Collective effects are stronger at lower energies W. Panovsky’s article in BEAM LINE Dashed line: ℒ~ 𝐸 𝐶𝑀 2 𝐸 𝐶𝑀 =100 MeV: ℒ~ 10 26 − 10 29 cm-2s-1

DANE 𝐸 +/− =0.51 GeV 𝐿=5.3⋅ 10 32 cm-2s-1 A low-energy electron-positron ring-ring collider 𝐸 +/− =0.51 GeV 𝐿=5.3⋅ 10 32 cm-2s-1

BABAR Search “Search for hadronic decays of a light Higgs boson in the radiative decay”, PRL 107, 221803 (2011)

BABAR Search M = 500 MeV 10k events/10 MeV Low statistics at low energies M = 500 MeV 10k events/10 MeV

Mass Range of Current Interest Need low-energy high-luminosity e+e- collider to cover range of interest Very asymmetric e+e- collider

Very Asymmetric Collider High-quality low-energy electron beam from a linac + High-quality high-energy positron beam stored in a ring = Small 𝑠=4 𝐸 + 𝐸 − ~4 GeV e+ ~100 MeV e-

Ring-Ring Collider, e.g. SuperKEK-B High energy High current High brightness High luminosity e+ e- E GeV 4 7 f MHz 248.5 I A 3.6 2.6 z mm 6 5 x/y nm/pm 3.2/8.64 4.6/12.9 x*/y* 32/0.27 25/0.30 x*/y* m/nm 10/48 11/62 x/y 0.0028/0.088 0.0012/0.081 L cm-2s-1 8  1035

Energy Recovery Linac Electrons pick energy up during acceleration and then deposit it back during deceleration with >99.9% efficiency Electrons from an energy-recovery linac High energy efficiency (determined by injector/dump energy) Relatively low current High brightness Cornell ERL project E GeV 5 f GHz 1.3 I A 0.1 z mm 0.6 x/y pm 31/31 xN/yN m 0.3/0.3

Linac-Ring Collider ERL size increased by a factor of 10 for visibility

Why Asymmetric Linac-Ring? Positrons stored in a ring High energy of ~3-5 GeV High current of ~2-3 A Small beam size High rigidity Electrons from an energy-recovery linac High energy efficiency Low energy for 𝑠 <1 GeV Relatively large current for a linac of ~100 mA Low rigidity but can be disrupted much stronger than a stored beam Combination meets physics and detection requirements

Key Collider Parameters Luminosity assuming matched beam sizes 𝐿= 𝑁 + 𝑁 − 𝑓 𝑐 4𝜋 𝜎 𝑥 ∗ 𝜎 𝑦 ∗ Beam-beam tune shift for stored positrons: number of oscillations due to focusing by electron beam 𝜉 𝑦+ = 𝑟 𝑒 𝑁 − 𝛽 𝑦+ ∗ 2𝜋 𝛾 + 𝜎 𝑦− ∗ 𝜎 𝑥− ∗ + 𝜎 𝑦− ∗ ≲0.08 Disruption parameter for electrons from linac: related to number of oscillations 𝑛 due to focusing by positron beam 𝐷 𝑦− = 2 𝑟 𝑒 𝑁 + 𝜎 𝑧+ 𝛾 − 𝜎 𝑦+ 𝜎 𝑥+ + 𝜎 𝑦+ ≲20 , 𝑛≈ 𝐷 𝑦− 4 Hour-glass effect 𝑅 𝑡 𝑥 , 𝑡 𝑦 = −∞ ∞ 𝑑𝑡 𝜋 exp − 𝑡 2 1+ 𝑡 2 / 𝑡 𝑥 2 1+ 𝑡 2 / 𝑡 𝑦 2 −1/2 , 𝑡 𝑦 ≈ 𝛽 𝑦 ∗ 𝜎 𝑧 Crossing angle 𝑅 𝐿 ≈ 1+ tan 𝜙 ⋅ 𝜎 𝑧 / 𝜎 𝑥 ∗ 2 −1/2

Hour-Glass Effect No hour glass effect 𝛽 ∗ ≳ 𝜎 𝑧 ( 𝜎 𝑧 ≡ bunch length) Strong hour-glass effect 𝛽 ∗ ≪ 𝜎 𝑧 e- bunch   e+ bunch e- bunch   e+ bunch 𝛽 ∗ ~ 𝜎 𝑧

Disruption Parameter Focusing of the linac beam by the opposing beam Electron 𝐷 𝑦− ≡ positron bunch length / electron beam-beam focal length Number of electron oscillations 𝑛= 𝐷 𝑦− /4 May cause emittance growth of the linac May cause kink instability of the stored beam Disruption parameters of up to 300 have been considered fro aggressive designs but typically 𝐷 𝑦− ≲20

Disruption Parameter Continued Y. Hao et al., “Beam beam study of ERL based eRHIC”, arXiv:1410.6000v1 [physics.acc-ph] (2014) 𝐷 𝑦− =27 𝐷 𝑦− =150

Problem due to Low Energy of Electrons How well can a linac-ring do at the limit of positron beam-beam tune shift? SuperKEK-B LER Cornell ERL Linac-Ring e+ e- E GeV 4 5 0.1 f MHz 248.5 1300 I A 3.6 2.6 0.095 z mm 6 0.6 1 x/y pm/pm 3200 / 8.64 31 / 31 850 / 850 5100 / 5100 xN/yN m/m 25 / 0.07 0.3 / 0.3 6.7 / 6.7 1 / 1 x*/y* 32 / 0.27 6 / 6 x*/y* 10 / 0.048 2.3 / 2.3 x/y 0.0028 / 0.088 0.08 / 0.08 Dx/Dy 1530 / 1530 Rh.-g. 0.41 L cm-2s-1 8  1035 Could be 3.4  1034 but

Proposed Solution: SuperKEK-B-Type Scheme Collide bunches at an angle and over-focus Keep high luminosity from the waist Eliminate negative dynamical effect from the rest of the bunch Then what enters into the equations for disruption parameter, beam-beam tune shift, and hour-glass effect are effective positron bunch length: 𝜎 𝑧+ = 𝜎 𝑥+ / tan 𝜃 effective positron current: 𝐼 + = 𝐼 + 𝜎 𝑧+ / 𝜎 𝑧+ Luminosity restored by focusing stronger in the vertical plane

SuperKEK-B-Type Scheme Assuming crossing angle of 10 𝑚𝑟𝑎𝑑 ⇒ 𝜎 𝑧+ =0.2 𝑚𝑚, 𝐼 + =120 𝑚𝐴 SuperKEK-B LER Cornell ERL Linac-Ring e+ e- E GeV 4 5 0.1 f MHz 248.5 1300 I A 3.6 2.6 0.095 z mm 6 0.6 1 x/y pm/pm 3200 / 8.64 31 / 31 850 / 85 5100 / 255 xN/yN m/m 25 / 0.07 0.3 / 0.3 6.7 / 0.67 1 / 0.05 x*/y* 32 / 0.27 6 / 0.6 1 / 0.2 x*/y* 10 / 0.048 2.3 / 0.23  mrad 83 10 x/y 0.0028 / 0.088 0.016 / 0.016 Dx/Dy 1.7 / 17 Rh.-g. 0.9 Rc.-a. 0.7 L cm-2s-1 8  1035 Achievable 1.7  1034

Magnetized Beam Electron beam born in solenoid field has two transverse canonical emittances Large one associated with beam size Small one associated with Larmor motion Space charge sets a limit only on the large emittance Emittance ratio can reach a factor of ~100 Magnetized beam property is routinely used in electron cooling Round beam after acceleration can be transformed to flat Y.-E Sun et al., Phys. Rev. ST Accel. Beams 7, 123501 (2004). An ERL for a magnetized beam is under development at JLab in the context of Jefferson Lab Electron-Ion Collider (JLEIC)

Possible Interaction Region Layout Experiment with detect a single high-energy photon Azimuthal angle cover of only 30% needed Detection requirements are conceptually similar to but much simpler than forward detection system that is being developed for JLEIC 𝐴 ′ p (top view in GEANT4) e low-Q2 electron detection and Compton polarimeter Forward hadron spectrometer ZDC

Discussion Considered case of 𝑠 = 1.3 GeV but can reach lower 𝑠 by lowering linac energy; L = const if I- ~ 1/Ee  I- ~ 1 A at Ee ~ 10 MeV Considered only high-level parameters, more detailed study is needed Currently considering a ring-ring scheme with electrons and positrons moving in the same direction: luminosity is suppressed by low CM energy but beams can be quite small

Conclusion Linac-ring collider for dark matter search in the region of photon mass of 0.1-1 GeV with L > 1034 cm-2s-1 can be built on the basis of an electron ERL and a positron storage ring The proposed design is based on proven concepts SuperKEK-B type beam crossing scheme Energy-recovery linac Magnetized electron beam Linac-ring is perhaps a relatively low cost option for such a collider with two orders of magnitude higher luminosity than other colliders of similar energy