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Search for dark photons from neutral meson decays in p plus p and d plus Au collisions at root s(NN)=200 GeV
- Adare, A. (author)
- Afanasiev, S. (author)
- Aidala, C. (author)
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- Ajitanand, N. N. (author)
- Akiba, Y. (author)
- Akimoto, R. (author)
- Al-Bataineh, H. (author)
- Al-Ta'ani, H. (author)
- Alexander, J. (author)
- Alfred, M. (author)
- Andrews, K. R. (author)
- Angerami, A. (author)
- Aoki, K. (author)
- Apadula, N. (author)
- Aphecetche, L. (author)
- Appelt, E. (author)
- Aramaki, Y. (author)
- Armendariz, R. (author)
- Asai, J. (author)
- Asano, H. (author)
- Aschenauer, E. C. (author)
- Atomssa, E. T. (author)
- Averbeck, R. (author)
- Awes, T. C. (author)
- Azmoun, B. (author)
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- Yoon, I. (author)
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- (creator_code:org_t)
- 2015
- 2015
- English.
- In: Physical Review C (Nuclear Physics). - 0556-2813. ; 91:3
- Journal article (peer-reviewed)
Abstract
Subject headings
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- The standard model (SM) of particle physics is spectacularly successful, yet the measured value of the muon anomalous magnetic moment (g - 2)mu deviates from SM calculations by 3.6 sigma. Several theoretical models attribute this to the existence of a "dark photon," an additional U(1) gauge boson, which is weakly coupled to ordinary photons. The PHENIX experiment at the Relativistic Heavy Ion Collider has searched for a dark photon, U, in pi(0), eta -> gamma e(+)e(-) decays and obtained upper limits of O(2 x 10(-6)) on U-gamma mixing at 90% C.L. for the mass range 30 < m(U) < 90 MeV/c(2). Combined with other experimental limits, the remaining region in the U-gamma mixing parameter space that can explain the (g - 2)(mu) deviation from its SM value is nearly completely excluded at the 90% confidence level, with only a small region of 29 < m(U) < 32 MeV/c(2) remaining.
Subject headings
- NATURVETENSKAP -- Fysik -- Subatomär fysik (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Subatomic Physics (hsv//eng)
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- art (subject category)
- ref (subject category)
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- Adare, A.
- Afanasiev, S.
- Aidala, C.
- Ajitanand, N. N.
- Akiba, Y.
- Akimoto, R.
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- Al-Bataineh, H.
- Al-Ta'ani, H.
- Alexander, J.
- Alfred, M.
- Andrews, K. R.
- Angerami, A.
- Aoki, K.
- Apadula, N.
- Aphecetche, L.
- Appelt, E.
- Aramaki, Y.
- Armendariz, R.
- Asai, J.
- Asano, H.
- Aschenauer, E. C ...
- Atomssa, E. T.
- Averbeck, R.
- Awes, T. C.
- Azmoun, B.
- Babintsev, V.
- Bai, M.
- Baksay, G.
- Baksay, L.
- Baldisseri, A.
- Bandara, N. S.
- Bannier, B.
- Barish, K. N.
- Barnes, P. D.
- Bassalleck, B.
- Basye, A. T.
- Bathe, S.
- Batsouli, S.
- Baublis, V.
- Baumann, C.
- Bazilevsky, A.
- Beaumier, M.
- Beckman, S.
- Belikov, S.
- Belmont, R.
- Ben-Benjamin, J.
- Bennett, R.
- Berdnikov, A.
- Berdnikov, Y.
- Bhom, J. H.
- Bickley, A. A.
- Black, D.
- Blau, D. S.
- Boissevain, J. G ...
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- Borel, H.
- Boyle, K.
- Brooks, M. L.
- Broxmeyer, D.
- Bryslawskyj, J.
- Buesching, H.
- Bumazhnov, V.
- Bunce, G.
- Butsyk, S.
- Camacho, C. M.
- Campbell, S.
- Caringi, A.
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- Chang, W. C.
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- Churyn, A.
- Chvala, O.
- Cianciolo, V.
- Citron, Z.
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