The first observation of the concurrent production of two mesons in proton-nucleus collisions is presented. The analysis is based on a proton-lead ( ) data sample recorded at a nucleon-nucleon center-of-mass energy of 8.16 TeV by the CMS experiment at the CERN LHC and corresponding to an integrated luminosity of . The two mesons are reconstructed in their decay channels with transverse momenta and rapidity . Events where one of the mesons is reconstructed in the dielectron channel are also considered in the search. The process is observed with a significance of 5.3 standard deviations. The measured inclusive fiducial cross section, using the four-muon channel alone, is . A fit of the data to the expected rapidity separation for pairs of mesons produced in single (SPS) and double (DPS) parton scatterings yields and , respectively. This latter result can be transformed into a lower bound on the effective DPS cross section, closely related to the squared average interparton transverse separation in the collision, of at 95% confidence level. © 2024 CERN, for the CMS Collaboration2024CERN 
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                    This content will become publicly available on January 1, 2026
                            
                            Inference of the Mass Composition of Cosmic Rays with Energies from 1018.5 to 1020  eV Using the Pierre Auger Observatory and Deep Learning
                        
                    
    
            We present measurements of the atmospheric depth of the shower maximum , inferred for the first time on an event-by-event level using the surface detector of the Pierre Auger Observatory. Using deep learning, we were able to extend measurements of the distributions up to energies of 100 EeV ( ), not yet revealed by current measurements, providing new insights into the mass composition of cosmic rays at extreme energies. Gaining a 10-fold increase in statistics compared to the fluorescence detector data, we find evidence that the rate of change of the average with the logarithm of energy features three breaks at , , and , in the vicinity to the three prominent features (ankle, instep, suppression) of the cosmic-ray flux. The energy evolution of the mean and standard deviation of the measured distributions indicates that the mass composition becomes increasingly heavier and purer, thus being incompatible with a large fraction of light nuclei between 50 and 100 EeV. Published by the American Physical Society2025 
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                            - PAR ID:
- 10581226
- Author(s) / Creator(s):
- ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »
- Publisher / Repository:
- American Physical Society
- Date Published:
- Journal Name:
- Physical Review Letters
- Volume:
- 134
- Issue:
- 2
- ISSN:
- 0031-9007
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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