Abstract

The quantum interference between the decays of entangled neutral kaons is studied in the process ϕ → KSKLπ+ππ+π, which exhibits the characteristic Einstein-Podolsky-Rosen correlations that prevent both kaons to decay into π+π at the same time. This constitutes a very powerful tool for testing at the utmost precision the quantum coherence of the entangled kaon pair state, and to search for tiny decoherence and CPT violation effects, which may be justified in a quantum gravity framework.

The analysed data sample was collected with the KLOE detector at DAΦNE, the Frascati ϕ-factory, and corresponds to an integrated luminosity of about 1.7 fb1, i.e. to about 1.7 × 109ϕ → KSKL decays produced. From the fit of the observed ∆t distribution, being ∆t the difference of the kaon decay times, the decoherence and CPT violation parameters of various phenomenological models are measured with a largely improved accuracy with respect to previous analyses.

The results are consistent with no deviation from quantum mechanics and CPT symmetry, while for some parameters the precision reaches the interesting level at which — in the most optimistic scenarios — quantum gravity effects might show up. They provide the most stringent limits up to date on the considered models.

Details

Title
Precision tests of quantum mechanics and CPT symmetry with entangled neutral kaons at KLOE
Author
Babusci, D. 1 ; Berlowski, M. 2 ; Bloise, C. 1 ; Bossi, F. 1 ; Branchini, P. 3 ; Budano, A. 4 ; Cao, B. 5 ; Ceradini, F. 6 ; Ciambrone, P. 1 ; Curciarello, F. 7 ; Czerwiński, E. 8 ; D’Agostini, G. 9 ; D’Amico, R. 9 ; Danè, E. 1 ; De Leo, V. 9 ; De Lucia, E. 1 ; De Santis, A. 1 ; De Simone, P. 1 ; Di Cicco, A. 10 ; Di Domenico, A. 9   VIAFID ORCID Logo  ; Diociaiuti, E. 1 ; Domenici, D. 1 ; D’Uffizi, A. 1 ; Fantini, A. 11 ; Fantini, G. 9 ; Fermani, P. 1 ; Fiore, S. 12 ; Gajos, A. 8 ; Gauzzi, P. 9 ; Giovannella, S. 1 ; Graziani, E. 3 ; Ivanov, V. L. 13 ; Johansson, T. 5 ; Kang, X. 14 ; Kisielewska-Kamińska, D. 8 ; Kozyrev, E. A. 13 ; Krzemien, W. 2 ; Kupsc, A. 5 ; Lukin, P. A. 13 ; Mandaglio, G. 15 ; Martini, M. 16 ; Messi, R. 17 ; Miscetti, S. 1 ; Moricciani, D. 1 ; Moskal, P. 8 ; Passeri, A. 3 ; Patera, V. 18 ; Perez del Rio, E. 9 ; Santangelo, P. 1 ; Schioppa, M. 7 ; Selce, A. 19 ; Silarski, M. 8 ; Sirghi, F. 20 ; Solodov, E. P. 13 ; Tortora, L. 3 ; Venanzoni, G. 21 ; Wiślicki, W. 2 ; Wolke, M. 5 

 Laboratori Nazionali di Frascati dell’INFN, Frascati, Italy (GRID:grid.463190.9) (ISNI:0000 0004 0648 0236) 
 National Centre for Nuclear Research, Warsaw, Poland (GRID:grid.450295.f) (ISNI:0000 0001 0941 0848) 
 INFN Sezione di “Roma Tre”, Roma, Italy (GRID:grid.470220.3) 
 Dipartimento di Matematica e Fisica dell’Università “Roma Tre”, Roma, Italy (GRID:grid.470220.3); INFN Sezione di “Roma Tre”, Roma, Italy (GRID:grid.470220.3) 
 Uppsala University, Department of Physics and Astronomy, Uppsala, Sweden (GRID:grid.8993.b) (ISNI:0000 0004 1936 9457) 
 Dipartimento di Matematica e Fisica dell’Università “Roma Tre”, Roma, Italy (GRID:grid.8993.b); INFN Sezione di “Roma Tre”, Roma, Italy (GRID:grid.470220.3) 
 Dipartimento di Fisica dell’Università della Calabria, Arcavacata di Rende, Italy (GRID:grid.7778.f) (ISNI:0000 0004 1937 0319); INFN Gruppo collegato di Cosenza, Arcavacata di Rende, Italy (GRID:grid.6045.7) (ISNI:0000 0004 1757 5281) 
 Jagiellonian University, Institute of Physics, Cracow, Poland (GRID:grid.5522.0) (ISNI:0000 0001 2162 9631) 
 Dipartimento di Fisica dell’Università “Sapienza”, Roma, Italy (GRID:grid.7841.a); INFN Sezione di Roma, Roma, Italy (GRID:grid.470218.8) 
10  Dipartimento di Matematica e Fisica dell’Università “Roma Tre”, Roma, Italy (GRID:grid.463190.9); INFN Sezione di “Roma Tre”, Roma, Italy (GRID:grid.470220.3) 
11  Dipartimento di Fisica dell’Università “Tor Vergata”, Roma, Italy (GRID:grid.463190.9); INFN Sezione di Roma “Tor Vergata”, Roma, Italy (GRID:grid.470219.9) 
12  ENEA, Department of Fusion and Technology for Nuclear Safety and Security, Frascati, Italy (GRID:grid.5196.b) (ISNI:0000 0000 9864 2490); INFN Sezione di Roma, Roma, Italy (GRID:grid.470218.8) 
13  Budker Institute of Nuclear Physics, Novosibirsk, Russia (GRID:grid.418495.5) (ISNI:0000 0001 0790 5468); Novosibirsk State University, Novosibirsk, Russia (GRID:grid.4605.7) (ISNI:0000000121896553) 
14  Laboratori Nazionali di Frascati dell’INFN, Frascati, Italy (GRID:grid.463190.9) (ISNI:0000 0004 0648 0236); China University of Geosciences, School of Mathematics and Physics, Wuhan, China (GRID:grid.503241.1) (ISNI:0000 0004 1760 9015) 
15  Dipartimento di Scienze Matematiche e Informatiche, Scienze Fisiche e Scienze della Terra dell’Università di Messina, Messina, Italy (GRID:grid.4605.7); INFN Sezione di Catania, Catania, Italy (GRID:grid.470198.3) (ISNI:0000 0004 1755 400X) 
16  Laboratori Nazionali di Frascati dell’INFN, Frascati, Italy (GRID:grid.463190.9) (ISNI:0000 0004 0648 0236); Dipartimento di Scienze e Tecnologie applicate, Università “Guglielmo Marconi”, Roma, Italy (GRID:grid.440899.8) (ISNI:0000 0004 1780 761X) 
17  Dipartimento di Fisica dell’Università “Tor Vergata”, Roma, Italy (GRID:grid.440899.8); INFN Sezione di Roma “Tor Vergata”, Roma, Italy (GRID:grid.470219.9) 
18  Dipartimento di Scienze di Base ed Applicate per l’Ingegneria dell’Università “Sapienza”, Roma, Italy (GRID:grid.470220.3); INFN Sezione di Roma, Roma, Italy (GRID:grid.470218.8) 
19  Dipartimento di Matematica e Fisica dell’Università “Roma Tre”, Roma, Italy (GRID:grid.6045.7); INFN Sezione di “Roma Tre”, Roma, Italy (GRID:grid.470220.3) 
20  Laboratori Nazionali di Frascati dell’INFN, Frascati, Italy (GRID:grid.463190.9) (ISNI:0000 0004 0648 0236); Horia Hulubei National Institute of Physics and Nuclear Engineering, Măgurele, Romania (GRID:grid.443874.8) (ISNI:0000 0000 9463 5349) 
21  INFN Sezione di Pisa, Pisa, Italy (GRID:grid.470216.6) 
Pages
59
Publication year
2022
Publication date
Apr 2022
Publisher
Springer Nature B.V.
e-ISSN
10298479
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2648629676
Copyright
© The Author(s) 2022. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.