Neutral K, Λ and production in K−p and K+p interactions at 32 GeV/c

Beillière, P.; Cochet, C.; Dumont, J. J.; Miller, D. B.; Faccini, M.L.; Fenjuk, A.B.; Gensch, U.; Henri, Victor; Johnstad, H.; Kaufmann, H. H.; Kozlovsky, E. A.; Laurent, J.; Meyer, A.; Moiseev, A.M.; Mosca, L.; Nikolaenko, V.; Nowak, H.; Smadja, G.; Tarasevich, S. V.; Triantis, F. A.; Windmolders, R.

doi:10.1016/0550-3213(75)90631-8

Cited by 22 publications

(1 citation statement)

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“…Important data is also collected at the Super Proton Synchrotron (SPS), the pre-accelerator of the LHC and the Relativistic Heavy-Ion Collider (RHIC). Data on π and K collisions is only available at energies up to tens of GeV in √ s [311][312][313][314][315] because interactions can only be studied with secondary beams. Since QCD is flavour-blind and the hadron multiplicity increases fast with √ s, the flavour and number of valence quarks becomes less important at high energies [312], however, it would be desirable to confirm this experimentally.…”

Section: Leveraging Colliders To Inform Hadronic Interaction Modelsmentioning

confidence: 99%

Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers

Coleman,

Eser,

Mayotte

et al. 2022

Preprint

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Pin down the shower energy observable to use μ as a composition-only Reduce hadronic uncertainties interaction model E threshold (TBD) Other messengers Galactic * μ / em separation † * depending on analysis progress † depending on detector configuration• At least one next-generation experiment needs to be able to make high-precision measurements to explore new particle physics and measure particle rigidity on an event-by-event basis. Of the planned next-generation experiments, GCOS is the best positioned to meet this recommendation.• As a complementary effort, experiments with sufficient exposure ( 5 × 10 5 km 2 sr yr) are needed to search for Lorentz-invariance violation (LIV), SHDM, and other BSM physics at the Cosmic and Energy Frontiers, and to identify UHECR sources at the highest energies.• Full-sky coverage with low cross-hemisphere systematic uncertainties is critical for astrophysical studies. To this end, next generation experiments should be space-based or multi-site. Common sites between experiments are encouraged.• Based on the productive results from inter-collaboration and inter-disciplinary work, we recommend the continued progress/formation of joint analyses between experiments and with other intersecting fields of research (e.g., magnetic fields).• The UHECR community should continue its efforts to advance diversity, equity, inclusion, and accessibility. It also needs to take steps to reduce its environmental impacts and improve open access to its data to reduce the scientific gap between countries.vi

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