HEP Research and Technology Division
OverviewDOE/HEP PI Meeting 2018
Glen Crawford
Research and Technology Division Director
Office of High Energy Physics
Office of Science, U.S. Department of Energy
Bottom-line Up Front
Great things are happening!
Important and exciting results across the portfolio
Great future leaders are revealed through Early
Career Awards!
Their ideas are supported by the ECA, with 91 HEP
Awards since 2010
Great new ideas in both science and technology
are emerging from the community, generating
interest and excitement!
We are working on ways to support these new ideas
DOE/HEP PI Meeting 2018 2
FY 2019 Budget Request Highlights
Energy Frontier: Actively engage in successful LHC program and HL-LHC upgrades The High-Luminosity Large Hadron Collider (HL-LHC) ATLAS & CMS detector upgrades (new
MIE starts) and the HL-LHC Accelerator Upgrade Project are together considered one of P5’s highest priority large projects
The U.S. will continue to play a leadership role in LHC discoveries by remaining actively engaged in analysis of world’s highest energy particle collider data
Intensity Frontier: Support establishing U.S.-hosted world-leading neutrino program LBNF/DUNE is P5’s highest priority U.S.-hosted large project, FY19 investments in far-site civil
construction crucial to enable scheduled delivery of contributions from international partners
Support Short-Baseline Neutrino (SBN) program at Fermilab, DUNE prototype R&D efforts at CERN, and continued funding for PIP-II project to upgrade the Fermilab Accelerator Complex
Cosmic Frontier: Advance our understanding of dark matter and dark energy P5 recommended complementary suite of projects to search for dark matter candidates and
study dark energy; request supports full planned profile for LZ, SuperCDMS-SNOLAB, DESI
3DOE/HEP PI Meeting 2018
HEP Research Priorities
Broadly speaking, focus will be (not
necessarily in priority order):
Research activities critical to executing the
upcoming P5 projects;
Supporting initial data taking and analysis from
new experiments coming on-line;
Continued analysis of ongoing experiments highly
recommended to address the P5 science drivers;
and
Supporting young investigators
DOE/HEP PI Meeting 2018 4
DOE HEP Research Priorities: Snapshot
Energy Frontier
Analysis of LHC Run 2 data
Contribute to operational responsibilities and complete “Phase I” upgrades
Scientific support for HL-LHC program
Intensity Frontier
Neutrino Program
Support ProtoDUNE, LBNF/DUNE, and PIP-II
Implement Fermilab Short-Baseline Neutrino Program and Intermediate Neutrino Program
NOvA, T2K/SK, Minerva, MicroBooNE data analysis
Muon Program: Complete Mu2e, take data with Muon g-2
Heavy Flavor Program: take and analyze data with Belle-II
Cosmic Frontier
Dark Matter: Scientific support for G2 experiments (in fabrication)
Dark Energy: DES analysis; scientific support for LSST and DESI (in fabrication)
Continue science planning for CMB-S4
Accelerator R&D
Focus on outcomes and capabilities that will dramatically improve cost effectiveness for mid-term and far-term accelerators
Hosting workshops to develop and implement R&D plan following P5 and GARD panels
Detector R&D
Developing process to identify highest priority R&D activities for current phase of implementing P5
Long-term “high-risk” R&D with potential for wide applicability and/or high-impact
“Blue-Sky” scientific research on innovative technologies not already in contention for implementation in future DOE HEP projects
HEP Theory
Maintain an overall “thriving” program as per P5
DOE/HEP PI Meeting 2018 5
See PM parallel session talks Wed/Thu
FY 2018 Early Career Awards: Univ.
Thomas Faulkner, University of Illinois New perspectives on QFT and gravity from quantum entanglement
Alexie Leauthaud-Harnett, University of California, Santa Cruz Exploiting Synergies Between Lensing and BAO Surveys for Improved
Cosmological Constraints
Themis Mastoridis, California Polytechnic State University Optimal Design of Radio Frequency Algorithms and Models for Next
Generation Accelerators
Benjamin Safdi, University of Michigan Particle Dark Matter Across Scales
Hee-Jong Seo, Ohio University Optimal and robust reconstruction of BAO, redshift-space distortions
and the Alcock-Paczynski effect
David Simmons-Duffin, Caltech Precision Computations in Strongly Coupled Conformal Field Theories
Rachel P. Yohay, Florida State University Probing New Physics with Tau Leptons using the CMS Detector
DOE/HEP PI Meeting 2018 6
FY 2018 Early Career Awards: Labs
Artur Apresyan, FNAL Exploring the Lifetime Frontier with New Detectors and New Searches
Daniel Bowring, FNAL Microwave Single-Photon Sensors for Dark Matter Searches and
Precision Neutrino Measurements
Daniel A. Dwyer, LBNL Improving Neutrino Detection in DUNE with Pixel Sensors
Michael Kagan, SLAC Exploring the Higgs Sector at the Energy Frontier with Bottom Quarks,
Machine Learning, and the Upgraded ATLAS Pixel Detector
Aritoki Suzuki, LBNL Development of high throughput techniques for SC microfabrication,
assembly and deployment for future high energy physics experiments
Kazuhiro Terao, SLAC GPU/FPGA Accelerated Deep Learning Technique Development for
Discovering Physics in Liquid Argon Time Projection Chambers
Javier Tiffenberg, FNAL Towards table-top neutrino detectors: A 10 kg Skipper-CCD
experiment
7
HEP Program Highlights
DOE/HEP PI Meeting 2018 8
Energy Frontier: LHC, ATLAS, and CMS
U.S. ATLAS represents ~19% of the international ATLAS Collaboration 41 universities, 4 national labs (Argonne,
Brookhaven, Lawrence Berkeley, SLAC)
Brookhaven is host lab for U.S. ATLAS
U.S. CMS represents ~29% of the international CMS Collaboration 53 universities, 1 national lab
Fermilab is host lab for U.S. CMS
States hosting members of the U.S. LHC experimental program
The Large Hadron Collider at CERN is the centerpiece of the U.S. Energy Frontier program
Large Hadron Collider Tunnel ATLAS Detector CMS Detector
DOE/HEP PI Meeting 2018 9
HL-LHC Accelerator Upgrades:Enabling U.S. Science Participation
10
DOE contribution:10 cold mass (Nb3Sn)
assemblies • 4 each for
ATLAS & CMS interaction regions
• 2 spares
DOE contribution:Hollow e-Lens Components (under discussion)
DOE contribution:20 Crab Cavities (16 + 4 spares)or: 10 Crab cavities & Hollow e-Lens Components
See M Procario talk (next)
EF Highlight: ttH Production
April 2018 results from ATLAS and CMS on Higgs production in association with a top quark pair
ATLAS combined result observes 4.2σsignificance (3.8σexpected)
Phys. Rev. D 97, 072003
CMS combined result observes 5.2σsignificance (4.2σexpected)
Accepted for Phys. Rev. Lett. [arXiv:1804.02610]
DOE/HEP PI Meeting 2018 11
IEEE Milestone for Tevatron Technology
On Nov. 13, the Institute of Electrical and Electronics Engineers (IEEE) recognized the technological innovations driven by the Tevatron with a prestigious IEEE Milestone Award for the development of the accelerator’s superconducting magnets During construction, 95% percent of the world's niobium-titanium
production went into the Tevatron's 774 superconducting magnets
DOE/HEP PI Meeting 2018 12
“The first large-scale use of superconducting magnets enabled the construction of the Tevatron. By 1985, the Tevatron achieved energy above 1 Tera electron-volt (TeV) in proton-antiproton collisions, making it the most powerful particle collider in the world until 2009. The Tevatron construction established the superconducting wire manufacturing infrastructure that made applications such as Magnetic Resonance Imaging (MRI) viable.”
Future Colliders
DOE coordinating with international community towards development of the next collider program U.S. looks forward to a decision this year by Japan to host the ILC as an international project
Global strategy for circular collider awaits 2020 European Strategy Update for Particle Physics
Interest from HEP community to pursue R&D studies for future collider options Circular collider: DOE efforts focused on high-field magnet technology to enable higher energy
ILC: DOE efforts focused on cost reduction R&D, e.g., nitrogen treatment in SRF cavities has potential for up to 10% cost reductions in 3-5 years, up to 15% in 5-10 years
Near-term priorities aim to support the LHC program including HL-LHC upgrades
High-Q0
(e.g. LCLS-II)
High-Q0; High-Eacc
(e.g. ILC)
SRF cavity:
Nitrogen Treatment R&D
DOE/HEP PI Meeting 2018 13
Intensity Frontier Program
Intensity Frontier experiments address the P5 Science Drivers through intense beams and sensitive detectors
Exploring the unknown through precision measurements: Muon g-2, Muon-to-Electron Conversion Experiment
(Mu2e), Belle II, K0TO
Identify the new physics of dark matter: Heavy Photon Search
Pursuing the physics associated with neutrino mass: NOvA, Daya Bay, MINERvA, Super-K, T2K ongoing
Ramping up Fermilab Short-Baseline Neutrino Program (MicroBooNE, SBND, ICARUS)
Preparing to host world-leading neutrino program with the Long-Baseline Neutrino Facility and Deep Underground Neutrino Experiment (LBNF/DUNE)
Muon g-2
NOvA
Belle II
DOE/HEP PI Meeting 2018 14
Collaboration News
André Rubbia
Phone Call
May 29, 2015
Long-Baseline Neutrino Facility and Deep Underground Neutrino Experiment
IllinoisSouthDakota Long-Baseline Neutrino Facility
IllinoisSouthDakota Long-Baseline Neutrino Facility
P5 recommended Long-Baseline Neutrino Facility (LBNF) as the centerpiece of a U.S.-hosted world-leading neutrino program LBNF will produce the world’s most intense neutrino
beam, send it 800 miles through the earth to DUNE
Strong support within the U.S. Government and many interested potential global partners
International DUNE collaboration includes: Over 1,100 collaborators from 176 institutions, 31 countries
Proton Improvement Plan II (PIP-II) will provide increased proton beam intensity (>1 MW) for LBNF
DOE/HEP PI Meeting 2018 15
Proton Improvement Plan II (PIP-II)
The P5 report recommended that PIP-II proceed immediately in order to provide increased proton beam intensity (of > 1 megawatt) for LBNF Replace the existing 50 year old linear accelerator with a higher power; one
powered by superconducting radiofrequency cavities
Supports longer-term physics research goals by providing increased beam power and high reliability for future experiments at Fermilab, including LBNF/DUNE
Old Fermilab Linac enclosure
New Fermilab Linac enclosure
DOE/HEP PI Meeting 2018 16
See M Procario talk (next)
IF Highlight: COHERENT Observes CEvNS
COHERENT experiment uses the world’s smallest neutrino detector to search for coherent elastic neutrino-nucleus scattering (CEνNS) 14.6-kg CsI[Na] scintillator operating at Oak Ridge National
Laboratory’s Spallation Neutron Source (SNS)
43 years after the first theoretical prediction, COHERENT observed CEvNS at a 6.7σ confidence level “Observation of coherent elastic neutrino-nucleus scattering”
published in Science, August 3, 2017
Characteristic signatures in energy and time, predicted by the Standard Model for this process, are observed in high signal-to-background conditions
DOE/HEP PI Meeting 2018 17
IF Highlight: First Collisions at Belle II
Belle II collaboration includes over 750 researchers from 25 countries and regions Includes a dozen U.S. Universities and Laboratories
U.S. Belle II project delivered key components of imaging Time-Of-Propagation (iTOP) and Klong-Muon (KLM) detector upgrade Received DOE Project Management Achievement
Award for delivering components ahead of schedule and under budget
Belle II aims to collect 50x the data of Belle over 10 years, using the 40x luminosity improvement of SuperKEKB
April 26: First collisions at SuperKEKB, after successfully storing electron and then positron beams in March 2018
DOE/HEP PI Meeting 2018 18
IF Highlight: SBN Far Detector Installation
ICARUS cold vessels now installed at Fermilab! Completed trans-Atlantic trip in July 2017
First cold vessel installed August 9, 2018
Second cold vessel installed August 14, 2018
Planning for data-taking in 2019
DOE/HEP PI Meeting 2018 19
Cosmic Frontier Program I
Cosmic Frontier experiments address the P5 science drivers using naturally occurring cosmic phenomena
In addition to NSF and NASA partnerships, most experiments and projects have international partners or contributions and some also have private contributions
Study dark energy’s role in the accelerating expansion of the universe through staged suite of complementary surveys Enables precision measurements that differentiate between
cosmological constant, modification to gravity, or new fields
Fast, wide area imaging surveys scan large volumes and catch dynamic events like supernovae: Dark Energy Survey (DES) operating, Large Synoptic Survey Telescope (LSST) 3-billion pixel camera in fabrication
Deep, high accuracy spectroscopic surveys study dim, more distant objects: eBOSS operating, Dark Energy Spectroscopic Instrument (DESI) in fabrication
Study inflation in the early universe using its imprint on the cosmic microwave background (CMB) South Pole Telescope 3G is operating, planning for P5-
recommended next-generation CMB Stage 4 experiment underway
AAAC Conceptual Design Team (CDT) developed strawman design (2017), Lab tech. development and pre-Project Design Group (pPDG) studies ongoing
DOE/HEP PI Meeting 2018 20
Cosmic Frontier Program II
Staged suite of dark matter direct detection experiments use multiple technologies to search for WIMP, Axion particles First-generation experiments produced world’s most sensitive
searches
P5-recommended 2nd generation experiments are advancing
ADMX-G2 axion search is operating; LZ and SuperCDMS-SNOLAB WIMP search projects in fabrication
Planning for small project(s) to address new priority science areas to search for dark matter
Pursue the physics associated with neutrino mass Dark Energy and CMB experiments also place unique constraints on
the sum of neutrino masses
Explore the unknown through cosmic- and gamma-ray experiments Perform indirect searches for dark matter and antimatter
Study fundamental physics properties such as breakdown of Lorentz invariance & high energy acceleration mechanisms
Space-based Fermi/GLAST & AMS and ground-based HAWC are currently operating
DOE/HEP PI Meeting 2018 21
Y1 galaxy clustering & weak lensing
CF Highlight: DES Y1 Results
DES studies Dark Energy via survey of 300 million galaxies, 3,000 supernovae with 570-megapixel Dark Energy Camera on Blanco telescope in Chile Planned 5 year ops. began Aug. 2013; extended through Dec. ‘18
Cosmology results from DES Year 1 data Aug. 2017: Galaxy clustering & weak lensing; competitive with Planck
Dec. 2017: Baryon Acoustic Oscillation (BAO) to z=1
Jan. 2018: Data Release 1; first 3 yrs. of survey data
Over 150 papers: most distant supernova, new Milky Way dwarf satellites to constrain dark matter, & more…
DOE/HEP PI Meeting 2018 22
DES Y1 produced largest map of dark matter in the Universe
Y1 BAO results
CF Highlight: ADMX-G2
Axion Dark-Matter eXperiment Generation 2 at U. Washington Uses a strong magnetic field and resonant cavity to convert dark matter
axions into detectable microwave photons
Selected as one of three G2 dark matter experiments following P5
Currently stepping through range 0.5 to 2 GHz (~ 2 to 8 micro-eV)
Dec. 2017 review of operations status (now led by Fermilab)
Results: May 2017: ADMX first experiment to reach Dine-Fischler-Srednicki-
Zhitnitsky (DFSZ) sensitivity limit for any axion mass range!
DOE/HEP PI Meeting 2018 23
Scientific AmericanJanuary 2018
Enabling Discovery though Advanced Technology R&D
Recent results:
Low-Loss Superconducting Radio-Frequency (SRF) Cavities using new processes developed by Fermilab Linac Coherent Light Source II (LCLS-II), under construction by Basic Energy
Sciences (BES), will be first beneficiary
Advances in laser-driven and beam-driven plasma wakefieldaccelerators Could produce high-gradient accelerators for future machines
Record current in high-temperature superconductors Could enable magnetic field levels that double existing particle collision
energies
DOE/HEP PI Meeting 2018 24
Advanced Technology R&D supports and advances research at all three experimental Frontiers
Fosters cutting-edge research in the physics of particle beams, accelerator R&D, and particle detection
Three broad categories: Near- to mid-term directed R&D for facilities/technologies in support of current DOE projects
Mid-term, facility-inspired R&D focused on concepts or technologies to demonstrate feasibility
Long-term, proposal-driven research on the fundamental science to enable breakthroughs in size, cost, beam intensity, beam energy, and control
Theoretical and Computational Physics
Provides the mathematical, phenomenological, and computational framework to understand and extend our knowledge of the dynamics of particles and forces, and the nature of space and time
Theoretical research essential for proper interpretation and understanding of the experimental research activities in other HEP subprograms
Advanced computing tools necessary for designing, operating, and interpreting experiments and scientific simulations that enable experimental discovery research
QIS: First HEP QIS call for proposals complete, see next slide for details
Implementing the P5 strategy requires advancing computing infrastructure to handle the exponentially increasing data and computing needs Partnerships with Advanced Scientific Computing Research (ASCR)
are an important part of addressing HEP computing needs
HEP aims to optimally leverage DOE resources in developing future computing solutions to meet mission needs
Cross-cutting efforts aim to prepare for future of computing, especially Exascale facilities
DOE/HEP PI Meeting 2018 25
FY 2018 QIS FOA & Lab Announcement
Quantum Information Science Enabled Discovery (QuantISED) for High Energy Physics
Closed April 16, 2018 HEP received an enthusiastic response!
Objective: Forge new routes to scientific discovery along HEP mission and P5 science drivers, invoking interdisciplinary advances in the convergent field of QIS, and intersection with expertise, techniques, technology developed in HEP community
Topics:
A: High Energy Physics and QIS Research
B: Quantum Computing for HEP on current or future quantum computing systems
Track 1: Pioneering Pilots (open to Topics A or B)
Work scope: Novel concepts, test problems, design studies (TRL 1)
Award: $100k - $500k over 1-2 years
Track 2: HEP-QIS Consortia (Open to Topic A only)
Work scope: Address P5, small experiments, early research on tools (TRL 1-2)
Award: FOA 500k – $2M (FOA) or $1M - $4M (LAB) over 2-3 years
Public announcement of selected HEP QIS proposals in Sept!
DOE/HEP PI Meeting 2018 26
See L Chatterjee talk (Wed PM)
Accelerator Stewardship
Mission: Support fundamental accelerator science and technology development of relevance to many fields and to disseminate accelerator knowledge and training to the broad community of accelerator users and providers.
Improve access to national lab accelerator facilities Make resources and facilities, such as Brookhaven National
Laboratory’s Accelerator Test Facility II (ATF-II), available for industrial and for other U.S. government agency users and developers of accelerators and related technology
Develop innovative solutions to critical problems outside of the DOE Office of Science More performant, lower cost accelerators for medicine
1000x speedup of laser-based science tools
Accelerator tech. for Energy & Environmental applications
Broaden and strengthen the community Bringing accelerator scientists, application scientists, and
industrialists together to address high-impact challenges
DOE/HEP PI Meeting 2018 27
See E Colby talk Thu AM
P5 Implementation Planning
In addition to executing P5 recommended
projects, DOE/HEP has developed processes
to examine the research portfolio and guide
implementation
Balance small and large investments
Establish R&D milestones and goals
Examine new ideas
GARD Workshops
HEP Portfolio Review
Basic Research Needs Workshops
DOE/HEP PI Meeting 2018 28
Adv. Tech. R&D: Research Roadmaps
Following the release of the HEPAP Accelerator R&D Subpanel Report in April 2015, the General Accelerator R&D (GARD) Program has engaged its research community to address the Subpanel recommendations to develop research roadmaps for these thrust areas: Superconducting High Field Magnets
Produced the U.S. Magnet Development Program Plan
Advanced Accelerator Concepts
Laser-driven plasma wakefield acceleration (LWFA)
Particle-beam-driven plasma wakefield acceleration (PWFA)
Dielectric wakefield acceleration (DWFA)
Radiofreqency Acceleration Technology
Superconducting RF
Normal Conducting RF
RF Sources
Community-developed roadmaps include: Pressing challenges to be addressed to move the field forward
Prioritized milestones aligned to the most compelling science
DOE/HEP PI Meeting 2018 29
Roadmaps Summary
Technology R&D Roadmaps are already having an impact in the HEP program Laboratory and University communities are aligning their efforts to meet the roadmap goals
Technology R&D Subprogram is using the roadmaps to guide program implementation
Progress and alignment will be assessed in lab accelerator R&D comparative review this summer
Roadmaps have also identified opportunities for possible applications of HEP Technology R&D to other program offices in the Office of Science Discussions are underway for opportunities where investments would have broad benefits
DOE/HEP PI Meeting 2018 30
HEP Portfolio Review
Portfolio Review assessed 13 currently operating HEP-supported experiments and prioritized their impact on P5 science drivers: 4 Tiers, from absolutely essential to “less effective”
HEP will prioritize ongoing support for top-Tier(s)
U.S. contributions to LHC experiments also examined, with generally high praise and a few comments
No DOE action will be taken in response to Portfolio Review recommendations without discussing with domestic and international partners Specific DOE guidance to experiments in response to
portfolio review recommendations will be sent in September 2018
DOE/HEP PI Meeting 2018 31
Basic Research Needs Workshops (BRNs)
SC’s Office of Basic Energy Sciences initiated this approach with the Basic Research Needs to Assure a Secure Energy Future workshop in October 2002. This resulted in a comprehensive, 420-page report that identified 37 Proposed Research Directions.
Numerous (~20) subsequent topically-focused BRNs have helped to define directions and make the case for major new efforts such as Energy Frontier Research Centers and Innovation Hubs
While there are some variations and there has been some evolution, many BRNs have involved:
Production of a Technology Perspectives Factual Document prior to the workshop
Definition of a set of Priority Research Directions that address the technology R&D challenges
Definition of a set of Science Grand Challenges that, if solved, might result in transformational changes
DOE/HEP PI Meeting 2018 32
BRN Process and Structure
Targeted topics defined by, and workshop charge issued by, SC program office
Attendance is limited and by invitation
Participants will have considerable work to do before, during, and after the meeting
Workshop Chair and Co-Chairs develop agenda and select panel leads (with program office input)
Typical structure: Opening plenary sessions, panel breakout sessions that develop priority research directions, closing plenary session, and extended writing session – draft report completed before departure!
Prompt output: final report released typically 60-90 days after the workshop
DOE/HEP PI Meeting 2018 33
BRN Impacts
BRN reports are expected to serve as reference documents with a long shelf life, and to be readily accessible
Post-workshop outreach activities often include communication of the results to the broader community by co-chairs and the SC program, and briefings by federal staff to other interested federal parties (within and beyond DOE)
BRNs may, individually or collectively, serve as the basis for subsequent funding opportunities. Examples:
An FY2007 FOA on Basic Research for Advanced Nuclear Energy Systems was based directly on the corresponding BRN, stating specifically that “The workshop report is a current source of information and summarizes the interests of BES.”
The original FY2009 solicitation for the Energy Frontier Research Centers (up to $100M/yr total) centered on the 11 BRNs that SC-BES had held to date
DOE/HEP PI Meeting 2018 34
HEP Basic Research Needs Workshops I
BRN workshop on New Opportunities for Dark Matter March 2017 community workshop held to determine scientifically
compelling areas to search and possible concepts for new experiments or studies
White Paper: https://arxiv.org/abs/1707.04591
Considering P5 recommendations and the current landscape, HEP will hold a BRN on Dark Matter in October 2018 to:
Identify priority science opportunities for new directions and areas of phase space that will provide significant science return and advancement.
Of these:
Which technology needs for which concepts for new small projects could be ready to go in the near term?
Which would be best carried out using DOE infrastructure and capabilities?
Co-Chairs have been identified and are starting to organize
Detector R&D is being considered for a future BRN workshop in 2019
DOE/HEP PI Meeting 2018 35
HEP Basic Research Needs Workshops II
BRN workshop on Compact Accelerators for Security and Medicine is in the planning stages for the coming year Focused on near-term applications
(3-5 years) of compact accelerator technologies to security and medical applications
Will identify high impact applications, technical gaps requiring basic R&D, and the primary barriers to technology adoption
Will identify required application-side R&D
Engage the other stakeholder federal agencies and provide a roadmap for near-term compact accelerator R&D, with particular attention given to technology transfer to industry
Will be by invitation only
DOE/HEP PI Meeting 2018 36
Image credit: LLNL
Image credit: 10.3390/ijms15069878
Summary
Great things are happening!
Important and exciting results across the portfolio
Great future leaders are revealed through Early
Career Awards!
Their ideas are supported by the ECA, with 91 HEP
Awards since 2010
Great new ideas in both science and technology
are emerging from the community, generating
interest and excitement!
We are working on ways to support these new ideas
DOE/HEP PI Meeting 2018 37
The Science Drivers of Particle Physics
The U.S. long-term strategy report identified five intertwined science drivers, compelling lines of inquiry that show great promise for discovery:
Use the Higgs boson as a new tool for discovery
Pursue the physics associated with neutrino mass
Identify the new physics of dark matter
Understand cosmic acceleration: dark energy and inflation
Explore the unknown: new particles, interactions, and physical principles
*2013
*2015
*2011
* Since 2011, three of the five science drivers havebeen lines of inquiry recognized with Nobel Prizes
DOE/HEP PI Meeting 2018 39
Enabling the Next Discovery
P5 identified 5 Science Drivers to address the scientific motivation in particle physics
Research Frontiers are useful categorization of experimental techniques and serve as the basis of the budget process
Research Frontiers arecomplementary No one Frontier addresses
all science drivers
Each Frontier provides adifferent approach toaddress science driver
Enables cross-checkingscientific results
DOE/HEP PI Meeting 2018 40
CMS HL-LHC Upgrade
DOE and NSF coordinating U.S. contributions with CERN and international partners on CMS Scope of the U.S. deliverables leverages expertise by U.S. scientists
3.8
*
*
Significant U.S. contributions
NSF
DOE NSF
DOE
DOE
NSF
= Significant
U.S. contributions
NSF
DOE
DOE/HEP PI Meeting 2018 41
ATLAS HL-LHC Upgrade
Similarly, U.S. ATLAS is defining the scope of its contributions to HL-LHC by leveraging interests and experience of U.S. groups, coordinating with international ATLAS
* Large forward rapidities, as described in the 2015 ATLAS HL-LHC scoping document (for the reference 275 MCHF CORE total cost scenario)
DOE Scope: Barrel Inner Tracker
(pixel & strip detector)
LAr Calorimeter front-end analog chip development
DAQ hardware (data flow elements)
NSF Scope: ‘Triggering’ at high
luminosities
Readout electronics for LAr, Tile, Muons
DOE/HEP PI Meeting 2018 42
LBNF/DUNE in South Dakota
Large-scale cryogenic vessel will house state-of-the-art neutrino detector one mile underground
215 ft.
61 ft.
Sanford Underground Research FacilityLead, South Dakota (U.S.)
55 ft.
Personfor Scale
4 cryostats at 10-ktons each
DOE/HEP PI Meeting 2018 43
Advancing Technology Towards LBNF/DUNE
Fermilab Short-Baseline Neutrino Program Resolve experimental anomalies in measured -spectrum, including search for sterile neutrino
Demonstrate the detector technology for DUNE
The largest liquid argon neutrino detector in the world, ICARUS was transported from Europe to Fermilab First major item of equipment to ship for the
international neutrino program
Far Detector – ICARUS (760-ton LAr)to be installed – Fall 2017
MiniBooNE
MicroBooNE(existing)
170-ton LAr
Fermilab Short-Baseline Neutrino Complex
DOE/HEP PI Meeting 2018 44
Program Advice and Coordination Formal advice (Federal Advisory Committee Act)
High Energy Physics Advisory Panel (HEPAP)
Jointly serves DOE and National Science Foundation (NSF)
2014: P5 long-term strategy report
2015: Accelerator R&D Subpanel report
Astronomy and Astrophysics Advisory Committee (AAAC)
Advises DOE, NSF, and NASA on selected issues of mutual interest within the fields of astronomy and astrophysics (e.g. CMB-S4 Conceptual Design Team)
Community input National Academies of Science: Astronomy and Astrophysics Decadal
Survey (New Worlds, New Horizons)
DOE Workshop reports, including Quantum Sensors, Accelerator R&D Roadmaps, Technology Connections, Basic Research Needs, etc.
International coordination CERN Council (LHC)
Governs CERN by defining its strategic programs, setting and following up its annual goals, and approving its budget
International Neutrino Council (LBNF/PIP-II)
International consulting body for DOE that facilitates high-level global coordination across the LBNF/PIP-II enterprise
Resources Review Board (DUNE)
Facilitates Fermilab’s coordination of resource-related matters for DUNE
DOE/HEP PI Meeting 2018 45
HEP FY 2019 Budget Request
Details
DOE/HEP PI Meeting 2018 46
FY 2019 President’s Budget Request
2019 President’s Budget Request for HEP is overlay of Administration, SC, P5 priorities SC: interagency partnerships, national laboratories, accelerator R&D, QIS
P5: preserve vision, modify execution
FY19 Budget Request reduces near-term science for P5-guided investments in mid- and long-term program “Building for Discovery” by supporting highest priority P5 projects to enable future program
Research support advances P5 science drivers and world-leading, long-term R&D in Advanced Technology, Accelerator Stewardship, and Quantum Information Science
Operations support enables world-class research at HEP User Facilities
The Administration and Congress support the overall P5 strategy FY19 House Mark for HEP: $1,004,510,000 ; FY19 Senate Mark for HEP: $1,010,000,000
DOE/HEP PI Meeting 2018 47
HEP Funding Category ($ in K)
FY 2017 Actual
FY 2018 Enacted
FY 2019 Request
FY 2019 vs.
FY 2018
Research 344,043 369,565 280,130 -89,435
Facilities/Operations 258,696 260,535 211,020 -49,515
Projects 222,261 277,900 278,850 +950
Total 825,000 908,000 770,000 -138,000
FY 2019 Funding by Subprogram
DOE/HEP PI Meeting 2018 48
HEP Funding Category ($ in K)
FY 2017 Actual
FY 2018 Enacted
FY 2019 Request
FY 19 vs. FY 18
Energy Frontier 154,274 190,938 181,232 -9,706
Intensity Frontier 242,924 246,768 200,170 -46,598
Cosmic Frontier 135,988 121,246 75,446 -45,800
Theoretical and Computational Physics
60,251 78,156 73,980 -4,176
Advanced Technology R&D 124,447 114,962 83,755 -31,207
Accelerator Stewardship 13,616 15,530 12,417 -3,113
Construction (Line Item) 93,500 140,400 143,000 +2,600
Total 825,000 908,000 770,000 -138,000
Research/Facilities/Project breakdown in following slides
Energy Frontier
Research: higher priority to support laboratory research activities to address the Higgs boson science driver, and to carry out the final analyses on data taken prior to LHC LS2 in 2019-20
Facility Operations: focus on commissioning of LHC ATLAS and CMS Detector Upgrade projects. Reduced support for compute nodes, data storage due to lower demand during LS2
Projects: increase supports new MIE starts for the HL-LHC ATLAS and HL-LHC CMS Detector Upgrade Projects and the planned increase for the HL LHC Accelerator Upgrade Project
DOE/HEP PI Meeting 2018 49
Energy Frontier($ in K)
FY 2017 Actual
FY 2018 Enacted
FY 2019 Request
FY 19 vs. FY 18
Research 72,268 79,530 56,119 -23,411
Facilities/Operations 52,771 54,340 44,309 -10,031
Projects 24,017 51,000 77,000 +26,000
LHC ATLAS Upgrade 8,500 - - ---
LHC CMS Upgrade 7,967 - - ---
HL-LHC Accelerator Upgrade 500 27,000 42,000 +15,000
HL-LHC ATLAS Upgrade 4,300 12,000 17,500 +5,500
HL-LHC CMS Upgrade 2,750 12,000 17,500 +5,500
SBIR/STTR 5,218 6,068 3,804 -2,264
Total 154,274 190,938 181,232 -9,706
Intensity Frontier
Research: higher priority to support laboratory research activities to address the neutrino mass and explore the unknown science drivers, and to carry out the early physics data analyses from Muon g-2, Belle II, SBN program and protoDUNE.
Facility Operations: activities will prioritize delivering the particle beams and providing experimental operations for ongoing experiments, including NOvA, SBN program, and Muon g-2. The Fermilab Accelerator Complex will be running at 75% of optimal levels.
Projects: focus on preliminary design and prototyping for the PIP-II project. OPC will continue for LBNF/DUNE for plant support costs.
DOE/HEP PI Meeting 2018 50
Intensity Frontier($ in K)
FY 2017 Actual
FY 2018 Enacted
FY 2019 Request
FY 19 vs. FY 18
Research 56,317 60,700 41,246 -19,454
Facilities/Operations 154,301 153,385 125,916 -27,469
Projects 24,569 24,100 26,000 +1,900
LBNF/DUNE - 1,000 1,000 ---
PIP-II 15,220 23,100 25,000 +1,900
Muon G-2 6,349 - - ---
SBIR/STTR 7,737 8,583 7,008 -1,575
Total 242,924 246,768 200,170 -46,598
Cosmic Frontier
Research: higher priority to support laboratory research activities to address the dark matter and dark energy science drivers, and to carry out the final data analyses on Cosmic Frontier experiments completing in FY 2019
Facility Operations: focus on the installation, commissioning and pre-operations activities for LSSTcam, DESI, LZ, and SuperCDMS-SNOLAB as these projects transition to operations
Projects: priority to support the fabrication and installation of the DESI, LZ, and SuperCDMS-SNOLAB projects. LSSTcam project funding will conclude as planned
DOE/HEP PI Meeting 2018 51
Cosmic Frontier($ in K)
FY 2017 Actual
FY 2018 Enacted
FY 2019 Request
FY 19 vs. FY 18
Research 45,990 49,892 31,506 -18,386
Facilities/Operations 13,353 16,310 11,320 -4,990
Projects 74,375 52,400 30,850 -21,550
LSSTcam 45,000 9,800 - -9,800
DESI 12,800 20,000 11,400 -8,600
LZ 12,500 14,100 14,450 +350
SuperCDMS 3,400 7,400 5,000 -2,400
SBIR/STTR 2,270 2,644 1,770 -874
Total 135,988 121,246 75,446 -45,800
Theoretical and Computational Physics
Theory Research: higher priority to research that addresses the neutrino mass science driver
Computational HEP: priority to advance computing research for HEP needs, and working with ASCR to optimize the high performance computing
Quantum Information Science: focus on research techniques and algorithms, foundational concepts relating particle physics and QIS, quantum computing for HEP experiments and modeling, development and use of specialized quantum controls and precision sensors
DOE/HEP PI Meeting 2018 52
Theoretical and Computational Physics($ in K)
FY 2017 Actual
FY 2018 Enacted
FY 2019 Request
FY 19 vs. FY 18
Research 55,713 75,303 71,280 -4,023
Theoretical Physics 44,848 43,000 32,753 -10,247
Computational HEP 7,924 8,500 7,435 -1,065
Quantum Information Science - 18,000 27,500 +9,500
Projects 2,300 - - ---
SBIR/STTR 2,238 2,853 2,700 -153
Total 60,251 78,156 73,980 -4,176
Advanced Technology R&D
General Accelerator R&D: priority to world-leading efforts supported at national laboratories
Directed Accelerator R&D: funding reduced as LARP goals will have been met
Detector R&D: near-term R&D activities will be ramped down
Facility Operations: focus on accelerator, test beam, and detector facilities at Fermilab. Funding for LBNL, SLAC supports highest priority research and fabrication activities. LBNL BELLA Second Beamline AIP begins, offset by completion of SLAC Sector 10 Injector Infrastructure AIP
Projects: focus on critical FACET-II infrastructure to be installed during shutdown for LCLS-II
DOE/HEP PI Meeting 2018 53
Advanced Technology R&D($ in K)
FY 2017 Actual
FY 2018 Enacted
FY 2019 Request
FY 19 vs. FY 18
Research 83,334 70,757 53,283 -17,474
GARD 44,357 44,500 36,544 -7,956
LARP 21,800 5,000 - -5,000
MAP 1,000 - - ---
Detector R&D 16,177 17,000 13,690 +9,500
Facilities/Operations 33,403 30,500 25,525 -4,975
Projects (FACET-II) 3,500 10,000 2,000 -8,000
SBIR/STTR 4,210 3,705 2,947 -758
Total 124,447 114,962 83,755 -31,207
Accelerator Stewardship
Research: priority will be given to long-term R&D for the science and technology needed to build future generations of accelerators.
Facility Operations: ATF II Upgrade AIP completion partially offset by the start of the 20TW CO2 Laser Upgrade AIP
DOE/HEP PI Meeting 2018 54
Accelerator Stewardship($ in K)
FY 2017 Actual
FY 2018 Enacted
FY 2019 Request
FY 19 vs. FY 18
Research 8,270 9,000 8,032 -968
Facilities/Operations 4,868 6,000 3,950 -2,050
SBIR/STTR 478 530 435 -95
Total 13,616 15,530 12,417 -3,113
Line Item Construction
LBNF/DUNE: funding will continue for far site civil
construction for the excavation of the caverns
Mu2e: FY 2019 will be last year of funding for the
project
PIP II: project engineering and design funding was
initiated in the FY 2018 enacted appropriation
DOE/HEP PI Meeting 2018 55
Construction (Line Item) ($ in K)
FY 2017 Actual
FY 2018 Enacted
FY 2019 Request
FY 19 vs. FY 18
LBNF/DUNE 50,000 95,000 113,000 +18,000
Mu2e 43,500 44,400 30,000 -14,400
PIP-II - 1,000 - -1,000
Total 93,500 140,400 143,000 +2,600
HEP MIE Project Status
DOE/HEP PI Meeting 2018 56
SubprogramTPC ($M)
CD Status
CD Date
INTENSITY FRONTIER
Long Baseline Neutrino Facility / Deep Underground Neutrino Experiment (LBNF/DUNE)
1,260 –1,860
CD-3A September 1, 2016
Proton Improvement Project (PIP-II) 653 - 928 CD-1 July 23, 2018
Muon g-2 44 CD-4 January 16, 2018
Muon-to-Electron Conversion Experiment (Mu2e) 274 CD-3 July 14, 2016
ENERGY FRONTIER
LHC ATLAS Detector Upgrade 33 CD-3 November 12, 2014
LHC CMS Detector Upgrade 33 CD-4A September 19, 2017
High-Luminosity LHC (HL-LHC) Accelerator Upgrade 208 - 252 CD-1/3A October 13, 2017
High-Luminosity LHC (HL-LHC) ATLAS Detector Upgrade 125-155 CD-0 April 13, 2016
High-Luminosity LHC (HL-LHC) CMS Detector Upgrade 125-155 CD-0 April 13, 2016
COSMIC FRONTIER
LUX-ZEPLIN (LZ) 56 CD-3 February 9, 2017
Super Cryogenic Dark Matter Search - SNOLAB (SuperCDMS-SNOLAB) 18.6 CD-2/3 May 2, 2018
Dark Energy Spectroscopic Instrument (DESI) 56 CD-3 June 22, 2016
Large Synoptic Survey Telescope Camera (LSSTcam) 168 CD-3 August 27, 2015
ADVANCED TECHNOLOGY R&D
Facility for Advanced Accelerator Experimental Tests II (FACET-II) 24.6 CD-2/3 June 8, 2018