| A | B | C | D | E | F | G | H | I | J | K | L | M | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | Please list White Papers, solicited or otherwise, that you are working on or involved with | Comments are now accepted for edits on individual tabs (see bottom of page). | |||||||||||
2 | As much information as possible is encouraged, but nothing is required | Conveners please contact Kristi or Tiffany for editing access. | |||||||||||
3 | The frontier conventions adopted are as follows: | EF = Energy Frontier, NF = Neutrino Frontier, CF = Cosmic Frontier, AF = Accelerator Frontier, TF = Theory Frontier, IF = Instrumentation Frontier | |||||||||||
4 | Inclusion in this database is meant to foster collaboration and does not constitue an official submission of your work to the Snowmass 2021 process. Please see snowmass21.org for official submission instructions. | RPF = Rare Processes and Precision Measurements Frontier, UF = Underground Facilities Frontier, CompF = Computation Frontier, CommF = Community Engagement Frontier | |||||||||||
5 | (Proposed) Title or Topic | arXiv Number | Endorsments Link | Is this being submitted on behalf of the Snowmass Early Career (SEC) group? | Is this White Paper solicited? | Submission Frontier(s) & Topical Group(s) | Main Topic(s)/Keywords | Coordinator Contact Email(s) | Collaboration | (Working) Document Link | Slack Channel | Notes | |
6 | Energy Frontier | ||||||||||||
7 | Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers | 2205.05845 | N | Y | CF07, EF | Cosmic Probes | Frank Schroeder, Fred Sarazin, Tonia Venters | N/A | Overleafs | — | CF07 Day Presentation | ||
8 | Synergy between astroparticle and collider physics | N | Y | EF, CF07 | Cosmic Probes | Hallsie Reno (CF07) | N/A | — | — | — | |||
9 | The International Linear Collider | 2203.07622 | N | N | CF01, EF, NF03, RF06, TF, AF03, IF, CommF07 | ILC Report | Michael Peskin | ILC | https://agenda.linearcollider.org/event/9135/ | -- | We are interested in including work on all aspects of e+e- Higgs/top factory physics. | ||
10 | The Forward Physics Facility: Sites, Experiments, and Physics Potential | 2109.10905 | N | N | CF, EF, NF, RF, TF | Far-Forward Physics | Felix King, Luis Anchordoqui | FPF | — | #fpf-whitepaper | CF07 Day Presentation | ||
11 | The Forward Physics Facility at the High-Luminosity LHC | 2203.05090 | Endorsements Sign-Up | N | N | CF, EF, NF, RF, TF, AF, IF | Far-Forward Physics | Jonathan Feng, Felix Kling, Juan Rojo, Hallsie Reno, Dennis Soldin | FPF | — | #fpf-whitepaper | CF07 Day Presentation | |
12 | Software and Computing for Small HEP Experiments | 2203.07645 | N | N | CF, EF, NF, RF, CompF | Computational Physics | Maria Elena Monzani | ||||||
13 | Detector and Beamline Simulation for Next-Generation High Energy Physics Experiments | 2203.07614 | N | N | CF, EF, NF, RF, IF, CompF02 | Computational Physics | Vincent Pascuzzi; Krzysztof Genser | ||||||
14 | Prompt electron andd tau neutrinos and antineutrinos in the forward region at the LHC | 2203.07212 | N | N | CF07, EF06, NF09 | Neutrino Probes— High Pseeudorapidity | Hallsie Reno | ||||||
15 | Strong CP Beyond Axion Direct Detection | 2203.07218 | N | N | CF02, EF09, TF08 | Strong CP Problem | Patrick Draper | ||||||
16 | Tau Neutrinos in the Next Decade: from GeV to EeV | 2203.05591 | N | N | CF07, EF09, NF03, TF11, IF, UF01 | Tau Neutrinos | Peter Denton | ||||||
17 | Probing the Electroweak Phase Transition with Exotic Higgs Decays | 2203.08206 | N | N | CF07, EF09 | Higgs Physics Program at LHC | Ke-Pan Xie | ||||||
18 | Higgs portal vector dark matter interpretation: review of Effective Field Theory approach and ultraviolet complete models | 2107.01252 | N | N | CF01, EF10 | Higgs-Portal Dark Matter | Mohamd Zaazoua | ||||||
19 | Portal Matter and Dark Sector Phenomenology at Colliders | 2202.02222 | N | N | CF01, EF10, TF07 | Dark Matter at Colliders | Thomas Rizzo | ||||||
20 | WIMP Dark Matter at High Energy Muon Colliders | 2203.07351 | N | N | CF01, EF10, TF07, AF04 | WIMP Dark Matter | Xing Wang | ||||||
21 | Neutrino Physics Frontier | ||||||||||||
22 | https://docs.google.com/spreadsheets/d/1ORQe5LYSaLQ7rsg7UihlD485cUDAxWlb9qZsOlgutIs/edit?usp=sharing | — | — | — | — | Kate Scholberg | — | — | — | Based off Neutrino Frontier Google Form | |||
23 | Tau Neutrinos in the Next Decade: from GeV to EeV | 2203.05591 | N | N | CF07, EF09, NF03, TF11, IF, UF01 | Tau Neutrinos | Peter Denton | (ABSTRACT) Tau neutrinos are the least studied particle in the standard model. The upcoming generation of experiments will provide unprecedented opportunities to increase our knowledge of this elusive particle. This whitepaper presents the state-of-the-art knowledge of the production and detection techniques and challenges across a broad range of experimental efforts. We also discuss the current status and future prospects for open questions both within the three-flavor paradigm and beyond. | |||||
24 | Theoretical tools for neutrino scattering: the interplay between lattice QCD, EFTs, nuclear physics, phenomenology, and neutrino event generators | 2203.09030 | N | NF06, TF11, CompF02 | Saori Pastore | (ABSTRACT) The focus of this whitepaper is on `Theoretical tools for neutrino scattering: the interplay between lattice QCD, EFTs, nuclear physics, phenomenology, and neutrino event generators'. This very broad topic has been divided into seven main sessions, namely, LQCD calculations for neutrino-nucleus scattering; Ab initio nuclear many-body studies for neutrino-nucleus scattering; Coherent elastic neutrino-nucleus scattering; Neutrino-induced shallow and deep inelastic scattering; The needs of the neutrino experimental program; Neutrino event generators; Neutrino interaction in dense matter. The need of this whitepaper is prompted by the many LOIs received across different frontiers on the topic of neutrino interactions. The goal of the whitepaper is to deliver a coherent and unified narrative of the theory requirements needed to advance the neutrino program. | |||||||
25 | Theory for neutrinoless double beta decay | N | NF06, TF11 (+ overlaps with TF, CompF, RPF) | Vincenzo Cirigliano | (ABSTRACT) The interpretation of current and future searches of neutrinoless double beta decay at the ton-scale and beyond in terms of mechanisms for lepton number violation is a multi-scale problem, involving the new physics, hadronic, and nuclear scales. Effective field theory(EFT), complemented by lattice QCD and nuclear many body methods, provides the bridge between the relevant scales. The goal of this WP is to provide a report on the status of the theory for neutrinoless double beta decay and a vision for the next ten years with an assessment of the capabilities required for progress. | ||||||||
26 | Future Advances in Photon-Based Neutrino Detectors | 2203.07479 | N | NF10, IF02 | Joshua Klein | (ABSTRACT) Large neutrino detectors that use photons as their primary detection mechanism have had enormous success. With the exception of radiochemical experiments, all major neutrino oscillation discoveries to date have been done with such detectors, whether they are monolithic and liquid-based, or segmented. Future photon-based detectors will require new approaches and enabling technologies, including hybrid Cherenkov/scintillation detectors, liquid noble detectors, the ability to load various isotopes, and new data acquisition electronics, simulation capabilities, and analysis techniques. In this White Paper we discuss these advances, including new target materials, fluors, loading techniques, fast timing, spectral photon sorting, and computing. | |||||||
27 | Neutrino Self-Interactions: A White Paper | N | NF03, NF05, TF11 (+ overlaps with TF) | Kevin Kelly | (ABSTRACT) Neutrino self-interactions have become a ripe topic for exploration over the last several years, and many different types of environments are sensitive to the possible interactions, from the laboratory, to astrophysics, to cosmology. We propose to compile the existing work on this topic into a coherent, digestible white paper. Additionally, we plan to outline some well-motivated frameworks for future studies in this field. | ||||||||
28 | Fixed-Target Searches for New Physics with O(10 GeV) Proton Beams at Fermi National Accelerator Laboratory | 2203.08102 | N | NF03, RF06, AF05 | Matthew Toups | (ABSTRACT) Proton beam dumps are prolific sources of mesons enabling a powerful technique to search for vector mediator coupling of dark matter to neutral pion and higher mass meson decays. In the next five years the PIP-II linac will be delivering up to 1 MW of proton power to the FNAL campus. This includes significant increase of power to the Booster Neutrino Beamline (BNB) which delivers 8 GeV protons to the Short Baseline Neutrino (SBN) detectors. By building a new dedicated beam dump target station, and using the SBN detectors, a greater than an order of magnitude increase in search sensitively for dark matter relative to the recent MiniBooNE beam dump search can be achieved. This modest cost upgrade to the BNB would begin testing models of the highly motivated relic density limit predictions. | |||||||
29 | Fixed-Target Searches for New Physics with O(1 GeV) Proton Beams at Fermi National Accelerator Laboratory | 2203.08079 | N | NF03, RF06, AF05 | Matthew Toups | (ABSTRACT; working) The focus of this white paper is to examine the sensitivities of new physics scenarios using a O(1 GeV) stopped-pion neutrino source at an upgraded Fermilab accelerator complex with the addition of the PIP-II linac with expected completion in 2027. Such a source combined with large detectors such as a reference 100-ton liquid argon scintillation detector would provide a powerful tool to search for accelerator-produced dark sector particles, new physics scenarios, and sterile neutrino searches via coherent elastic neutrino-nucleus scattering. Implementation of additional detectors such as an LSND-like scintillator detector could provide additional methods to search for sterile neutrinos. | |||||||
30 | White Paper on Cosmological Neutrinos | N | NF01, NF02, NF03, NF04, NF05, TF11 (+ overlaps with CF) | Evan Grohs | (ABSTRACT) The physics surrounding neutrino mass and neutrino interactions presents key research opportunities in elementary particle physics, both in theory and in experiment. Paralleling the developments in those fields, advances in observational astrophysics and cosmology promise unprecedented precision in the measurement of cosmological quantities. Since those quantities in many cases are shaped by how the physics of neutrinos plays out in the cauldron of the very early universe, and its aftermath, we can expect synergistic advances in both the fundamental physics of neutrinos and in cosmology. In what follows we point out several areas ripe for future investigation. | ||||||||
31 | Neutrino Physics at the Spallation Neutron Source Second Target Station | N | NF02, NF03, NF05, NF06, NF07, TF11, NF09 (+ overlaps with CF, IF, TF, AF) | Kate Scholberg | (ABSTRACT) The Oak Ridge National Laboratory (ORNL) Spallation Neutron Source (SNS) First Target Station (FTS), used by the COHERENT experiment, provides an intense and extremely high-quality source of pulsed stopped-pion neutrinos, with energies up to 50~MeV. Upgrades to the SNS are planned, including a Second Target Station (STS), which will approximately double the expected neutrino flux while maintaining quality similar to the FTS source. | ||||||||
32 | A Next-Generation Liquid Xenon Obsrvatory for Dark Matter and Neutrino Physics | 2203.02309 | N | N | CF01, NF04, RF03, IF08, UF03 | WIMP Parameter Space | Ibles Olcina | (ABSTRACT) A third generation (G3) two-phase liquid xenon TPC will not only be able to explore new regions of parameter space of dark matter, but also competitively search for some neutrino processes of interest, such as neutrinoless double beta decay (0ùúà2Œ≤). | |||||
33 | Fundamental properties of neutrinos from the point of view of cosmology | N | NF01, NF02, NF03, NF05, TF11 (+ overlaps with CF, TF, CompF) | Alexander Bonilla Rivera | (ABSTRACT) Neutrino mass is still an open question to be solved in the followingdecades. New experiments support the searches of predictions of amodel explaining the smallness of neutrino masses and the hierarchical structures of differences, and the presence of new Right Handed degrees of freedom of neutrinos. To test a model is unavoidable to solve before the ambiguity Dirac-Majorana for neutrino and hence to find the nature of new RH states. Cosmology observables can give us essential hints to see new degrees of freedom impact in face different observables. We will use Dirac particles protection from quantum gravity effects on global U(1) symmetries . We will see too this as Dirac neutrinos impact early universe anomaly UV composed model. | ||||||||
34 | Neutrinos and intergalactic communication problems. | N | NF01, NF02, NF04, NF05, NF06, NF07, TF11, NF09, NF10 | Paul Shapshak | (ABSTRACT) Signaling by advanced civilizations is evolving away from photon physics towards particle physics. Neutrinos specifically have greater penetrability compared to photons in interstellar and intergalactic medium. Coming to grips with how advanced civilizations may utilize neutrinos for communication involves understanding both neutrino physics and cosmology. These problems are embedded within a highly complex global background, within and beyond the Standard Model. Signal production and detection are central as well. | ||||||||
35 | High Energy Physics Opportunities Using Reactor Antineutrinos | 2203.07214 | N | NF09 | Bryce Littlejohn | (ABSTRACT) Reactor antineutrinos are broadly useful for probing neutrino properties, physics associated with neutrino mass, and BSM phenomena. Simultaneously, they offer a unique window into the inner workings and content of operating nuclear reactor cores. In this work, we will summarize how reactor antineutrinos can play a critical role in advancing the field of neutrino physics over the next decade. | |||||||
36 | Low Energy Physics in Liquid Argon | N | NF01, NF02, NF03, NF04, NF06, TF11, NF09, NF10 (+ overlaps with CF, TF, UF) | Kate Scholberg | Writeup based loosely on LEPLAr workshop contents | ||||||||
37 | Electron Scattering and Neutrino Physics: A Snowmass White Paper | 2203.06853 | N | NF06, TF11 | Vishvas Pandey | (ABSTRACT) Electron scattering provides key information to inform neutrino interaction models relevant to the current and future accelerator and atmospheric neutrino oscillation programs. Parity violating neutrino scattering also intersects with the low energy neutrino program (CEvNS). This white paper summarizes current and new efforts to apply knowledge from electron scattering to the neutrino sector. | |||||||
38 | Kilotonne-scale xenon detectors for new physics searches | N | NF03, NF05, NF10 (+ overlaps with IF) | David Moore | (ABSTRACT) Large detectors employing xenon are a leading technology in existing and planned searches for new physics, including searches for neutrinoless double beta decay (0νββ) and dark matter. While upcoming detectors will employ target masses of a tonne or more, further extending gas or liquid phase Xe detectors to the ktonne scale would enable extremely sensitive next-generation searches for rare phenomena. The key challenge to extending this technology to detectors well beyond the tonne scale is the acquisition of the Xe itself. We describe the motivation for extending Xe time projection chambers (TPCs) to the ktonne scale and possible avenues for Xe acquisition that avoid existing supply chains. If acquisition of Xe in the required quantities is successful, ktonne-scale detectors of this type could enable a new generation of experiments, including searches for 0νββ at half-life sensitivities as long as 10^30 yr. | ||||||||
39 | Neutrino Scattering Measurements on Hydrogen and Deuterium | N | NF01, NF02, NF03, NF05, NF06, TF11, NF10 (+ overlaps with TF, RPF) | Richard Hill, Thomas Junk | (ABSTRACT) Neutrino interaction uncertainties are a limiting factor in current and next generation experiments probing the fundamental physics of neutrinos, a unique window on physics beyond the Standard Model. Neutrino-nucleon scattering amplitudes are an important part of the neutrino interaction program. However, since all modern neutrino detectors are composed primarily of heavy nuclei, knowledge of elementary neutrino-nucleon amplitudes relies heavily on experiments from an earlier age whose statistical and systematic precision are insufficient for current needs. We are preparing a white paper in which we outline the motivation for measurements on hydrogen and/or deuterium that would improve this knowledge, and discuss options for making these measurements either at the DUNE near detector or at a dedicated facility. | ||||||||
40 | BSM effects on neutrino flavor | N | NF02, NF03 | Pilar Coloma | (ABSTRACT) This white paper will discuss the impact of BSM models on neutrino oscillations and on the flavor of ultra-high energy neutrinos. It will cover both theoretical and experimental aspects relevant for new physics searches for a variety of experiments spanning MeV to PeV energies. | ||||||||
41 | Searches for Baryon Number Violation in Neutrino Experiments | 2203.08771 | N | NF03, RF04 | Lisa Koerner | (ABSTRACT) This paper will summarize the experimental and theoretical aspects of baryon number violation searches performed in neutrino detectors. | |||||||
42 | A Gaseous Argon-Based Near Detector for DUNE to Enhance Physics Capabilities | N | NF01, NF03, NF06 (+ overlaps with IF) | Alysia Marino | (ABSTRACT) This document presents the concept and physics case for a magnetized gaseous argon-based tracking detector system for the DUNE Near Detector. A detector system like this is required in order for DUNE to reach its full physics potential. | ||||||||
43 | Neutrino Physics with a Large Selenium-82 Imaging Detector | 2203.08779 | N | NF05 | Alvaro E Chavarria | (ABSTRACT) Imaging sensors made from an ionization target layer of amorphous selenium (aSe) coupled to a silicon complementary metal-oxide-semiconductor (CMOS) active pixel array for charge readout are a promising technology for neutrino physics. The high spatial resolution in a solid-state target provides unparalleled rejection of backgrounds from natural radioactivity for zero-background spectroscopy of ùõΩùõΩ decay and electron neutrinos. This allows for a broad neutrino program that includes i) the search for neutrinoless ùõΩùõΩ decay, ii) solar neutrino spectroscopy, and iii) the search for sterile neutrinos with an intense electron-capture radioactive source. We present the scientific reach of a 10 tonne neutrino detector with the proposed technology based on our experimental understanding of the sensor performance. | |||||||
44 | Low Background kTon-Scale Liquid Argon Time Projection Chambers | 2203.08821 | N | N | CF01, NF10, IF08, UF01 | MeV-Scale Reach TPC | Chris Jackson, Eric Church | (ABSTRACT) With controls over radiopurity and some modifications to a detector similar to the DUNE Far Detector design we find that it is possible to increase sensitivity to low energy physics in a subsequent module. In particular, sensitivity to supernova and solar neutrinos can be enhanced with improved MeV-scale reach. Furthermore, sensitivity to Weakly-Interacting Massive Particle (WIMP) Dark Matter (DM) becomes competitive with the planned world program in such a detector. | |||||
45 | Neutrinos at ORNL | N | NF02, NF03, NF04, NF05, NF06, NF07, TF11, NF09, NF10 (+ overlaps with CF, IF, TF, AF) | Jason Newby | (ABSTRACT) Neutrino physics (and related) opportunities at ORNL (SNS, HFIR, NLDBD, supernova, detector R&D) | ||||||||
46 | Family Symmetry as a Possible Explanation for Lepton Masses and Mixing | N | NF02, NF03, TF11 | Biswajit Karmakar | (ABSTRACT) We discuss neutrino mass and mixing models based on family symmetries extended models with sterile neutrinos and 2HDM, 3HDM. We explore possible connections of such models with leptogenesis and dark matter. | ||||||||
47 | Theia: Summary of physics program | 2202.12839 | UF, NF, IF | Gabriel Orebi Gann | |||||||||
48 | The Forward Physics Facility: Sites, Experiments, and Physics Potential | 2109.10905 | N | N | CF, EF, NF, RF, TF | Far-Forward Physics | Felix King, Luis Anchordoqui | FPF | — | #fpf-whitepaper | CF07 Day Presentation | ||
49 | The Forward Physics Facility at the High-Luminosity LHC | 2203.05090 | Endorsements Sign-Up | N | N | CF, EF, NF, RF, TF, AF, IF | Far-Forward Physics | Jonathan Feng, Felix Kling, Juan Rojo, Hallsie Reno, Dennis Soldin | FPF | — | #fpf-whitepaper | CF07 Day Presentation | |
50 | Software and Computing for Small HEP Experiments | 2203.07645 | N | N | CF, EF, NF, RF, CompF | Computational Physics | Maria Elena Monzani | ||||||
51 | Detector and Beamline Simulation for Next-Generation High Energy Physics Experiments | 2203.07614 | N | N | CF, EF, NF, RF, IF, CompF02 | Computational Physics | Vincent Pascuzzi, Krzysztof Genser | ||||||
52 | CMB-S4 White Paper | 2203.08024 | N | N | CF, NF, IF | CMB-S4 Project | John Carlstrom | CMB-S4 | |||||
53 | The Sanford Underground Research Facility | 2203.08293 | N | N | CF, NF, RF, IF, CompF, UF, CommF | SURF | Jaret Heise | SURF | |||||
54 | The European Spallation Source neutrino Super Beam | 2203.08803 | N | N | CF, NF, RF, AF, UF | ESSvSB Design | Tamer Tolba | ESSvSB | |||||
55 | DUNE Physics Summary | 2203.06100 | N | N | CF01, NF, RF04 | DUNE BSM Results | Chris Marshall | ||||||
56 | CMB-HD: An Ultra-Deep, High-Resolution Millimeter Wave Survy over Half the Sky | 1906.10134 | N | N | CF, NF02 | CMB-HD Survey | Neelima Sehgal | CMB-HD | |||||
57 | A Strategy for Low-Mass Dark Matter Searches with Cryogenic Detectors in the SuperCDMS SNOLAB Facility | 2203.08463 | N | N | CF01, NF03, IF01, UF03 | SuperCDMS SNOLAB | Sunil Golwala | SuperCDMS | |||||
58 | The International Linear Collider | 2203.07622 | N | N | CF01, EF, NF03, RF06, TF, AF03, IF, CommF07 | ILC Report | Michael Peskin | ILC | |||||
59 | Introduction to a low-mass dark matter project, ALETHEIA: A Liquid hElium Time projection cHambEr In dArk matter | 2203.07901 | N | N | CF01, NF04, RF03, IF08, UF03 | ALETHEIA Project w.r.t. WIMPs | Junhui Liao | ||||||
60 | High-Energy and Ultra-High-Energy Neutrinos | 2203.08096 | Feedback & Endorsements | N | Y | CF07, NF04, TF09, IF10 | Cosmic Probes | Nepomuk Otte, Mauricio Bustamante, Steph Wissel, Hallsie Reno, Markus Ackermann, Lu Lu | N/A | ||||
61 | Synergy between cosmological and laboratory searches in neutrino physics | 2203.07377 | N | N | CF07, NF05, TF11 | Cosmic/Neutrino Frontier Intersection | Evan Grohs | ||||||
62 | Prompt electron and tau neutrinos and antineutrinos in the forward region at the LHC | 2203.07212 | N | N | CF07, EF06, NF09 | Neutrino Probes— High Pseudorapidity | Hallsie Reno | ||||||
63 | Passive low energy nuclear recoil detection with color centers - PALEOCCENE | 2203.05525 | N | N | CF01, NF10, IF03 | The PALEOCCENE Concept | Patrick Huber | PALEOCCENE | |||||
64 | Recoil imaging for dark matter, neutrinos, andd physics beyond the Standard Model | 2203.05914 | N | N | CF01, NF10, IF05 | Recoil Imaging | Ciaran O'Hare | ||||||
65 | High-pressure TPCs in pressurized caverns: opportunities in dark matter and neutrino physics | 2203.06262 | N | N | CF01, NF10, IF08, UF03 | TPCs in Lined Rock Caverns | Benjamin Monreal | ||||||
66 | Rare Processes & Precision Frontier | ||||||||||||
67 | The Forward Physics Facility: Sites, Experiments, and Physics Potential | 2109.10905 | N | N | CF, EF, NF, RF, TF | Far-Forward Physics | Felix King, Luis Anchordoqui | FPF | — | #fpf-whitepaper | CF07 Day Presentation | ||
68 | The Forward Physics Facility at the High-Luminosity LHC | 2203.05090 | Endorsements Sign-Up | N | N | CF, EF, NF, RF, TF, AF, IF | Far-Forward Physics | Jonathan Feng, Felix Kling, Juan Rojo, Hallsie Reno, Dennis Soldin | FPF | — | #fpf-whitepaper | CF07 Day Presentation | |
69 | Quantum Sensors for HEP Science— Interferometers Mechanics, Traps, and Clocks | 2203.07250 | N | N | CF, RF, IF01 | Quantum Sensors | Thomas Cecil | ||||||
70 | Software and Computing for Small HEP Experiments | 2203.07645 | N | N | CF, EF, NF, RF, CompF | Computational Physics | Maria Elena Monzani | ||||||
71 | Detector and Beamline Simulation for Next-Generation High Energy Physics Experiments | 2203.07614 | N | N | CF, EF, NF, RF, IF, CompF02 | Computational Physics | Vincent Pascuzzi, Krzysztof Genser | ||||||
72 | The Sanford Underground Research Facility | 2203.08293 | N | N | CF, NF, RF, IF, CompF, UF, CommF | SURF | Jaret Heise | SURF | |||||
73 | The European Spallation Source neutrino Super Beam | 2203.08803 | N | N | CF, NF, RF, AF, UF | ESSvSB Design | Tamer Tolba | ESSvSB | |||||
74 | A Next-Generation Liquid Xenon Obsrvatory for Dark Matter and Neutrino Physics | 2203.02309 | N | N | CF01, NF04, RF03, IF08, UF03 | WIMP Parameter Space | Rafael Lang | ||||||
75 | Introduction to a low-mass dark matter project, ALETHEIA: A Liquid hElium Time projection cHambEr In dArk matter | 2203.07901 | N | N | CF01, NF04, RF03, IF08, UF03 | ALETHEIA Project w.r.t. WIMPs | Junhui Liao | ||||||
76 | The NNBAR/HIBEAM Experimental Program | N | N | RF04 | Neutron Oscillations | Joshua Barrow | NNBAR | To follow | #neutron_oscillations | Collaborators welcome | |||
77 | Low-Scale Baryogenesis | N | N | RF04 | Baryogenesis | Joshua Barrow | N/A | To follow | #lowscalebaryogenesiswp | Collaborators welcome | |||
78 | DUNE Physics Summary | 2203.06100 | N | N | CF01, NF, RF04 | DUNE BSM Results | Chris Marshall | ||||||
79 | The International Linear Collider | 2203.07622 | N | N | CF01, EF, NF03, RF06, TF, AF03, IF, CommF07 | ILC Report | Michael Peskin | ILC | |||||
80 | Cosmic Frontier | ||||||||||||
81 | CMB-HD: An Ultra-Deep, High-Resolution Millimeter Wave Survy over Half the Sky | 1906.10134 | N | N | CF, NF02 | CMB-HD Survey | Neelima Sehgal | CMB-HD | |||||
82 | The Forward Physics Facility: Sites, Experiments, and Physics Potential | 2109.10905 | N | N | CF, EF, NF, RF, TF | Far-Forward Physics | Felix King, Luis Anchordoqui | FPF | — | #fpf-whitepaper | CF07 Day Presentation | ||
83 | The Forward Physics Facility at the High-Luminosity LHC | 2203.05090 | Endorsements Sign-Up | N | N | CF, EF, NF, RF, TF, AF, IF | Far-Forward Physics | Jonathan Feng, Felix Kling, Juan Rojo, Hallsie Reno, Dennis Soldin | FPF | — | #fpf-whitepaper | CF07 Day Presentation | |
84 | Early-Universe Model Building | 2203.06680 | N | N | CF, TF09 | Early Universe Phenomenology | Asher Berlin | ||||||
85 | Quantum Sensors for HEP Science— Interferometers Mechanics, Traps, and Clocks | 2203.07250 | N | N | CF, RF, IF01 | Quantum Sensors | Thomas Cecil | ||||||
86 | Software and Computing for Small HEP Experiments | 2203.07645 | N | N | CF, EF, NF, RF, CompF | Computational Physics | Maria Elena Monzani | ||||||
87 | Data Preservation for Cosmology | 2203.08113 | N | N | CF, TF09, CompF07 | Computational Physics | Stephen Bailey | ||||||
88 | Detector and Beamline Simulation for Next-Generation High Energy Physics Experiments | 2203.07614 | N | N | CF, EF, NF, RF, IF, CompF02 | Computational Physics | Vincent Pascuzzi Krzysztof Genser | ||||||
89 | CMB-S4 White Paper | 2203.08024 | N | N | CF, NF, IF | CMB-S4 Project | John Carlstrom | CMB-S4 | |||||
90 | The Sanford Underground Research Facility | 2203.08293 | N | N | CF, NF, RF, IF, CompF, UF, CommF | SURF | Jaret Heise | SURF | |||||
91 | The European Spallation Source neutrino Super Beam | 2203.08803 | N | N | CF, NF, RF, AF, UF | ESSvSB Design | Tamer Tolba | ESSvSB | |||||
92 | Dark Matter Direct Detection to the Neutrino Fog | 2203.08084 | Feedback & Endorsements | N | Y | CF01 | Particle-like Dark Matter | Rick Gaitskell, Cristiano Galbiati, Ben Loer, Prisca Cushman | N/A | — | #cf01-wp1-direct-detection-neutrino-floor | CF01 White Paper Google Drive | |
93 | The landscape of low-threshold dark matter direct detection in the next decade | 2203.08297 | N | Y | CF01 | Particle-like Dark Matter | Graham Giovanetti, Noah Kurinsky, Daniel McKinsey, Rouven Essig | N/A | — | #cf01-wp2-low-threshold-detection | CF01 White Paper Google Drive | ||
94 | Calibrations and backgrounds for dark matter direct detection | 2203.07623 | Feedback & Endorsements | N | Y | CF01 | Particle-like Dark Matter | Dan Baxter, Raymond Bunker, Sally Shaw, Shawn Westerdale | N/A | — | #cf01-wp3-calibration-backgrounds-direct | CF01 White Paper Google Drive | |
95 | Modeling, statistics, simulations, and computing needs for direct dark matter detection | 2203.07700 | N | Y | CF01, CompF | Particle-like Dark Matter | Yoni Kahn, Maria Elena Monzani, Kim Palladino | N/A | — | #cf01-wp4-comp-model-stats-direct | CF01 White Paper Google Drive | ||
96 | The landscape of cosmic-ray and high-energy-photon probes of particle dark matter | 2203.06894 | N | Y | CF01 | Particle-like Dark Matter | Tsuguo Aramaki, Stefano Profumo, Philip von Doetinchem | N/A | — | #cf01-wp5-cosmic-ray-and-photon-probes | CF01 White Paper Google Drive | ||
97 | Puzzling Excesses in Dark Matter Searches andd How to Resolve Them | 2203.06859 | N | Y | CF01, TF09 | Particle-like Dark Matter | Liang Yang, Rebecca Leane, Sam McDermott | N/A | — | #cf01-wp6-puzzling-excesses | CF01 White Paper Google Drive | ||
98 | Synergies between dark matter searches and multiwavelength/multimessnger astrophysics | 2203.06781 | N | Y | CF01 | Particle-like Dark Matter | Pat Harding, Shunsaki Horiuchi, Devin Walker | N/A | Overleaf | #cf01-wp7-dm-synergies-with-multiwavelength-astro | CF01 White Paper Google Drive | ||
99 | Ultraheavy particle dark matter | 2203.06508 | N | Y | CF01, TF08, IF01 | Particle-like Dark Matter | Nirmal Raj, Dan Carney | N/A | Overleaf | #cf01-wp8-ultraheavy-particle-dm | CF01 White Paper Google Drive; Contributor Google Sheet; Mailing list: SNOWMASS-UHDM@listserv.umd.edu | ||
100 | Hidden sectors and a multi-temperature universe | 2106.06494 | N | N | CF01, TF08 | Hidden Sectors | Amin Aboubrahim | ||||||