001009743 001__ 1009743
001009743 005__ 20250701125836.0
001009743 0247_ $$2doi$$a10.1103/PhysRevX.13.031004
001009743 0247_ $$2datacite_doi$$a10.34734/FZJ-2023-02963
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001009743 1001_ $$00000-0001-9439-3439$$aKaranth, S.$$b0
001009743 245__ $$aFirst Search for Axionlike Particles in a Storage Ring Using a Polarized Deuteron Beam
001009743 260__ $$aCollege Park, Md.$$bAPS$$c2023
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001009743 500__ $$aPublished by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Experimental Data available on Jülich DATA: https://doi.org/10.26165/JUELICH-DATA/HHNVQ3
001009743 520__ $$aBased on the notion that the local dark-matter field of axions or axionlike particles (ALPs) in our Galaxy induces oscillating couplings to the spins of nucleons and nuclei (via the electric dipole moment of the latter and/or the paramagnetic axion-wind effect), we establish the feasibility of a new method to search for ALPs in storage rings. Based on previous work that allows us to maintain the in-plane polarization of a stored deuteron beam for a few hundred seconds, we perform a first proof-of-principle experiment at the Cooler Synchrotron (COSY) to scan momenta near 970  MeV/c. This entails a scan of the spin-precession frequency. At resonance between the spin-precession frequency of deuterons and the ALP-induced electric dipole moment (EDM) oscillation frequency, there is an accumulation of the polarization component out of the ring plane. Since the axion frequency is unknown, the momentum of the beam and, consequently, the spin-precession frequency are ramped to search for a vertical polarization change that occurs when the resonance is crossed. At COSY, four beam bunches with different polarization directions are used to make sure that no resonance is missed because of the unknown relative phase between the polarization precession and the axion or ALP field. A frequency window of 1.5 kHz width around the spin-precession frequency of 121 kHz is scanned. We describe the experimental procedure and a test of the methodology with the help of a radio-frequency Wien filter located on the COSY ring. No ALP resonance is observed. As a consequence, an upper limit of the oscillating EDM component of the deuteron as well as its axion coupling constants are provided.
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001009743 536__ $$0G:(EU-Grant)694340$$asrEDM - Search for electric dipole moments using storage rings (694340)$$c694340$$fERC-2015-AdG$$x2
001009743 536__ $$0G:(EU-Grant)824093$$aSTRONG-2020 - The strong interaction at the frontier of knowledge: fundamental research and applications (824093)$$c824093$$fH2020-INFRAIA-2018-1$$x3
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001009743 7001_ $$00000-0003-3671-8877$$aStephenson, E. J.$$b1$$eCorresponding author
001009743 7001_ $$aChang, S. P.$$b2
001009743 7001_ $$0P:(DE-Juel1)131187$$aHejny, V.$$b3
001009743 7001_ $$aPark, S.$$b4
001009743 7001_ $$0P:(DE-Juel1)156288$$aPretz, J.$$b5
001009743 7001_ $$00000-0001-7941-6639$$aSemertzidis, Y. K.$$b6
001009743 7001_ $$0P:(DE-Juel1)131377$$aWirzba, A.$$b7
001009743 7001_ $$00000-0003-0126-3315$$aWrońska, A.$$b8
001009743 7001_ $$0P:(DE-Juel1)173899$$aAbusaif, F.$$b9
001009743 7001_ $$00000-0002-1100-1936$$aAggarwal, A.$$b10
001009743 7001_ $$0P:(DE-Juel1)164127$$aAksentev, A.$$b11
001009743 7001_ $$aAlberdi, B.$$b12
001009743 7001_ $$0P:(DE-Juel1)175125$$aAndres, A.$$b13
001009743 7001_ $$aBarion, L.$$b14
001009743 7001_ $$0P:(DE-Juel1)171927$$aBekman, I.$$b15
001009743 7001_ $$0P:(DE-HGF)0$$aBeyß, M.$$b16
001009743 7001_ $$0P:(DE-Juel1)164484$$aBöhme, C.$$b17
001009743 7001_ $$0P:(DE-Juel1)166211$$aBreitkreutz, B.$$b18
001009743 7001_ $$0P:(DE-Juel1)176948$$avon Byern, C.$$b19
001009743 7001_ $$00000-0003-2262-7077$$aCanale, N.$$b20
001009743 7001_ $$aCiullo, G.$$b21
001009743 7001_ $$aDymov, S.$$b22
001009743 7001_ $$0P:(DE-Juel1)171853$$aFröhlich, N.-O.$$b23
001009743 7001_ $$0P:(DE-Juel1)131164$$aGebel, R.$$b24
001009743 7001_ $$0P:(DE-Juel1)131170$$aGrigoryev, K.$$b25
001009743 7001_ $$0P:(DE-Juel1)131172$$aGrzonka, D.$$b26
001009743 7001_ $$0P:(DE-Juel1)162384$$aHetzel, J.$$b27
001009743 7001_ $$0P:(DE-Juel1)177857$$aJavakhishvili, O.$$b28
001009743 7001_ $$aJeong, H.$$b29
001009743 7001_ $$0P:(DE-Juel1)131201$$aKacharava, A.$$b30
001009743 7001_ $$0P:(DE-Juel1)131203$$aKamerdzhiev, V.$$b31
001009743 7001_ $$0P:(DE-Juel1)164243$$aKeshelashvili, I.$$b32
001009743 7001_ $$0P:(DE-Juel1)171526$$aKononov, A.$$b33
001009743 7001_ $$0P:(DE-Juel1)176945$$aLaihem, K.$$b34
001009743 7001_ $$0P:(DE-Juel1)131234$$aLehrach, A.$$b35
001009743 7001_ $$aLenisa, P.$$b36
001009743 7001_ $$aLomidze, N.$$b37
001009743 7001_ $$aLorentz, B.$$b38
001009743 7001_ $$00000-0002-7561-6366$$aMagiera, A.$$b39
001009743 7001_ $$0P:(DE-Juel1)131251$$aMchedlishvili, D.$$b40
001009743 7001_ $$aMüller, F.$$b41
001009743 7001_ $$0P:(DE-Juel1)131267$$aNass, A.$$b42
001009743 7001_ $$aNikolaev, N. N.$$b43
001009743 7001_ $$0P:(DE-Juel1)180911$$aPesce, A.$$b44
001009743 7001_ $$aPoncza, V.$$b45
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001009743 7001_ $$0P:(DE-Juel1)151369$$aSaleev, A.$$b48
001009743 7001_ $$00009-0000-5437-2836$$aShergelashvili, D.$$b49
001009743 7001_ $$0P:(DE-Juel1)176609$$aShmakova, V.$$b50
001009743 7001_ $$0P:(DE-Juel1)168362$$aShurkhno, N.$$b51
001009743 7001_ $$aSiddique, S.$$b52
001009743 7001_ $$0P:(DE-Juel1)172927$$aSlim, J.$$b53
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001009743 7001_ $$0P:(DE-Juel1)131342$$aStassen, R.$$b55
001009743 7001_ $$0P:(DE-Juel1)131349$$aStroeher, Hans$$b56$$ufzj
001009743 7001_ $$00009-0002-5975-6710$$aTabidze, M.$$b57
001009743 7001_ $$aTagliente, G.$$b58
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