2025-12-26 04:03 |
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2025-12-26 04:01 |
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Quirks Live in Cool Universes
/ Asadi, Pouya (UC, Santa Cruz) ; Kribs, Graham D. (Oregon U. ; CERN) ; Luty, Markus A. (UC, Davis, QMAP)
We demonstrate that cosmological observations place strong bounds on the reheat temperature $T_\text{RH}$ of the Standard Model (SM) in minimal models of `quirks' -- heavy fermions transforming under the SM gauge group together with a new non-Abelian gauge interaction with a confinement scale far below the mass of the fermions. [...]
CERN-TH-2025-243 ; arXiv:2512.20696.
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2025-12-25 04:33 |
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2025-12-24 04:52 |
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2025-12-24 04:52 |
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2025-12-20 04:04 |
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Probing scalar and pseudoscalar new physics using rare kaon decays
/ D'Ambrosio, G. (INFN, Naples) ; Iyer, A.M. (Indian Inst. Tech., New Delhi) ; Mahmoudi, F. (IP2I, Lyon ; CERN ; ENS, Lyon, Lab. Phys.) ; Neshatpour, S. (IP2I, Lyon)
Rare kaon decays provide sensitive tests of new physics. [...]
CERN-TH-2025-254 ; arXiv:2512.16903.
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2025-12-20 04:03 |
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2025-12-20 04:00 |
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The Physics of Herwig 7
/ Bellm, J. (Lund U.) ; Bewick, G. (Durham U., IPPP) ; Ferrario Ravasio, S. (Turin U. ; INFN, Turin) ; Gieseke, S. (KIT, Karlsruhe, TP) ; Grellscheid, D. (U. Bergen (main)) ; Kiebacher, S. (KIT, Karlsruhe, TP) ; Kirchgaeßer, P. (KIT, Karlsruhe, TP) ; Loshaj, F. (KIT, Karlsruhe, TP) ; Masouminia, M.R. (Durham U., IPPP) ; Nail, G. (U. Edinburgh (main)) et al.
We present the physics foundations and recent developments of Herwig 7, the modern successor of the original HERWIG and Herwig++ series. [...]
CERN-TH-2025-252 ; IPPP-25-57 ; HERWIG-2025-01 ; KA-TP-36-2025 ; MCNET-25-31 ; arXiv:2512.16645.
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2025-12-20 04:00 |
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2025-12-17 04:44 |
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The heavy quark-antiquark asymmetry in the variable flavor number scheme
/ Behring, A. (Garching, Max Planck Inst.) ; Blümlein, J. (DESY ; Dortmund U.) ; De Freitas, A. (Linz U., RISC) ; von Manteuffel, A. (Regensburg U.) ; Schneider, C. (Linz U., RISC) ; Schönwald, K. (CERN)
The twist-2 heavy-quark and antiquark distributions, as defined in the variable flavor number scheme, turn out to be different due to QCD corrections from three-loop onward. [...]
DESY 25--185 ; CERN--TH--2025--259 ; MPP--2025--227 ; RISC Report series 25--10 ; DESY 25-185 ; CERN-TH-2025-259 ; MPP-2025-227 ; RISC Report series 25-10 ; arXiv:2512.13508.
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