Neutron–Mirror-Neutron Oscillations: How Fast Might They Be?

Zurab Berezhiani and Luís Bento
Phys. Rev. Lett. 96, 081801 – Published 27 February 2006

Abstract

We discuss the phenomenological implications of the neutron (n) oscillation into the mirror neutron (n), a hypothetical particle exactly degenerate in mass with the neutron but sterile to normal matter. We show that the present experimental data allow a maximal nn oscillation in vacuum with a characteristic time τ much shorter than the neutron lifetime, in fact as small as 1 sec. This phenomenon may manifest in neutron disappearance and regeneration experiments perfectly accessible to present experimental capabilities and may also have interesting astrophysical consequences, in particular, for the propagation of ultra high energy cosmic rays.

  • Figure
  • Received 12 August 2005

DOI:https://doi.org/10.1103/PhysRevLett.96.081801

©2006 American Physical Society

Authors & Affiliations

Zurab Berezhiani1,* and Luís Bento2,†

  • 1Dipartimento di Fisica, Università di L’Aquila, I-67010 Coppito, AQ, Italy and Laboratori Nazionali del Gran Sasso, INFN, I-67010 Assergi, AQ, Italy
  • 2Faculdade de Ciências, Centro de Física Nuclear da Universidade de Lisboa, Universidade de Lisboa, Avenida Professor Gama Pinto 2, 1649-003 Lisboa, Portugal

  • *Electronic address: zurab.berezhiani@aquila.infn.it
  • Electronic address: lbento@cii.fc.ul.pt

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 96, Iss. 8 — 3 March 2006

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×