Abstract High energy collisions at the High-Luminosity Large Hadron Collider (LHC) produce a large number of particles along the beam collision axis, outside of the acceptance of existing LHC experiments. The proposed Forward Physics Facility (FPF), to be located several hundred meters from the ATLAS interaction point and shielded by concrete and rock, will host a suite of experiments to probe standard model (SM) processes and search for physics beyond the standard model (BSM). In this report, we review the status of the civil engineering plans and the experiments to explore the diverse physics signals that can be uniquely probed in the forward region. FPF experiments will be sensitive to a broad range of BSM physics through searches for new particle scattering or decay signatures and deviations from SM expectations in high statistics analyses with TeV neutrinos in this low-background environment. High statistics neutrino detection will also provide valuable data for fundamental topics in perturbative and non-perturbative QCD and in weak interactions. Experiments at the FPF will enable synergies between forward particle production at the LHC and astroparticle physics to be exploited. We report here on these physics topics, on infrastructure, detector, and simulation studies, and on future directions to realize the FPF’s physics potential.
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String Derived Z' Model at an Upgraded Superconducting Super Collider
The future of collider physics is under investigation. With the High Luminosity LHC program lasting
until the late 2030s, the next machine in the energy frontier is envisioned to appear in 30-40 years, which
may be too far into the future to sustain the field. In this paper we explore the physics potential of an
Upgraded Superconducting Super Collider (USSC). The Original Superconducting Super Collider (OSSC)
was planned to operate at 20 TeV beam energy, and with improved magnet technology and/or longer
tunnel, one may envision that it can be extended to 25-30 TeV beam energy. Given that the decision on
the OSSC construction took place in Autumn 1988 and it was planned to start operation in the 1996-1999
period, an USSC can be constructed 10-15 years from construction and fill the gap between the end of HL-LHC and the future envisioned machines. While the main mission of the USSC will be to test the Standard
Model and its electroweak and strongly interacting sectors, as a specific example we illustrate the invariant
mass distribution at NNLO in QCD for a 5 TeV Z′ in the string derived Z′ model.
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- Award ID(s):
- 2112025
- PAR ID:
- 10554563
- Publisher / Repository:
- Andromeda Conference Proceedings (ACP)
- Date Published:
- Journal Name:
- Andromeda Conference Proceedings
- ISSN:
- 2632-2714
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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- Free Publicly Accessible Full Text
-
Accepted Manuscript1.0
- Journal Article:
- https://doi.org/10.31526/BSM-2023.2
