544 research outputs found

    Evidence of a p-ϕ\phi bound state

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    The existence of a nucleon-ϕ\phi (N-ϕ\phi) bound state has been subject of theoretical and experimental investigations for decades. In this letter a re-analysis of the p-ϕ\phi correlation measured at the LHC is presented, using as input recent lattice calculations of the N-ϕ\phi interaction in the spin 3/2 channel obtained by the HAL QCD collaboration. A constrained fit of the experimental data allows to determine the spin 1/2 channel of the p-ϕ\phi interaction with evidence of the formation of a p-ϕ\phi bound state. The scattering length and effective range extracted from the spin 1/2 channel are f0(1/2)=(1.470.37+0.44(stat.)0.17+0.14(syst.)+i0.000.00+0.26(stat.)0.00+0.15(syst.))f_0^{(1/2)}=(-1.47^{+0.44}_{-0.37}(\mathrm{stat.})^{+0.14}_{-0.17}(\mathrm{syst.})+i\cdot0.00^{+0.26}_{-0.00}(\mathrm{stat.})^{+0.15}_{-0.00}(\mathrm{syst.})) fm and d0(1/2)=(0.370.08+0.07(stat.)0.03+0.03(syst.)+i 0.000.02+0.00(stat.)0.01+0.00(syst.))d_0^{(1/2)}=(0.37^{+0.07}_{-0.08}(\mathrm{stat.})^{+0.03}_{-0.03}(\mathrm{syst.})+i\cdot~0.00^{+0.00}_{-0.02}(\mathrm{stat.})^{+0.00}_{-0.01}(\mathrm{syst.})) fm, respectively. The corresponding binding energy is estimated to be in the range 14.756.614.7-56.6 MeV. This is the first experimental evidence of a p-ϕ\phi bound state

    Experimental test of Non-Commutative Quantum Gravity by VIP-2 Lead

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    Pauli Exclusion Principle (PEP) violations induced by space-time non-commutativity, a class of universality for several models of Quantum Gravity, are investigated by the VIP-2 Lead experiment at the Gran Sasso underground National Laboratory of INFN. The VIP-2 Lead experimental bound on the non-commutative space-time scale Λ\Lambda excludes θ\theta-Poincar\'e far above the Planck scale for non vanishing ``electric-like" components of θμν\theta_{\mu \nu}, and up to 6.91026.9 \cdot 10^{-2} Planck scales if they are null. Therefore, this new bound represents the tightest one so far provided by atomic transitions tests. This result strongly motivates high sensitivity underground X-ray measurements as critical tests of Quantum Gravity and of the very microscopic space-time structure.Comment: 13 pages, 2 figures. arXiv admin note: substantial text overlap with arXiv:2209.0007

    Strongest atomic physics bounds on Non-Commutative Quantum Gravity Models

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    Investigations of possible violations of the Pauli Exclusion Principle represent critical tests of the microscopic space-time structure and properties. Space-time non-commutativity provides a class of universality for several Quantum Gravity models. In this context the VIP-2 Lead experiment sets the strongest bounds, searching for Pauli Exclusion Principle violating atomic-transitions in lead, excluding the θ\theta-Poincar\'e Non Commutative Quantum Gravity models far above the Planck scale for non-vanishing θμν\theta_{\mu \nu} ``electric-like'' components, and up to 6.91026.9 \cdot 10^{-2} Planck scales if θ0i=0\theta_{0i} = 0.Comment: 7 pages, 2 figure

    VIP-2 —High-Sensitivity Tests on the Pauli Exclusion Principle for Electrons

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    The VIP collaboration is performing high sensitivity tests of the Pauli Exclusion Principle for electrons in the extremely low cosmic background environment of the underground Gran Sasso National Laboratory INFN (Italy). In particular, the VIP-2 Open Systems experiment was conceived to put strong constraints on those Pauli Exclusion Principle violation models which respect the so-called Messiah–Greenberg superselection rule. The experimental technique consists of introducing a direct current in a copper conductor, and searching for the X-rays emission coming from a forbidden atomic transition from the L shell to the K shell of copper when the K shell is already occupied by two electrons. The analysis of the first three months of collected data (in 2018) is presented. The obtained result represents the best bound on the Pauli Exclusion Principle violation probability which fulfills the Messiah–Greenberg rule

    High Precision Test of the Pauli Exclusion Principle for Electrons

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    The VIP-2 experiment aims to perform high precision tests of the Pauli Exclusion Principle for electrons. The method consists in circulating a continuous current in a copper strip, searching for the X radiation emission due to a prohibited transition (from the 2p level to the 1s level of copper when this is already occupied by two electrons). VIP already set the best limit on the PEP violation probability for electrons 12β2<4.7×1029\frac{1}{2} \beta^2 < 4.7 \times 10^{-29}, the goal of the upgraded VIP-2 (VIolation of the Pauli Exclusion Principle-2) experiment is to improve this result of two orders of magnitude at least. The experimental apparatus and the results of the analysis of a first set of collected data will be presented

    Search for a remnant violation of the Pauli exclusion principle in a Roman lead target

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    In this paper we report on the results of two analyses of the data taken with a dedicated VIP-Lead experiment at the Gran Sasso National Laboratory of the INFN. We use measurements taken in an environment that is especially well screened from cosmic rays, with a metal target made of “Roman lead” which is characterised by a low level of intrinsic radioactivity. The analyses lead to an improvement, on the upper bounds of the Pauli Exclusion Principle violation for electrons, which is more than one (four) orders of magnitude, when the electron-atom interactions are described in terms of scatterings (or close encounters) respectively
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