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Opening day
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Submission deadline
Submission of your abstract implies that you are willing to present the work as a poster or as a talk. Please indicate your preferred presentation type on the submission form. The convenors will review the abstracts after the submission deadline and, subject to space available, schedule the talks and posters.
Please note that before you can submit an abstract you must have created an account on this Lawrence Berkeley National Laboratory (LBNL) Indico instance, using the Login tab at the top of this page. After submitting the form you will receive a confirmation e-mail that includes a link which you must use to activate your account.
NOTE: All Indico instances worldwide are discrete, with their own sets of accounts, and therefore you must create an account on this LBNL site in order to be able to submit an abstract.
When creating your account, please pay particular attention to entering your Family and First names in the correct fields. Use correct capitalization for your names and affiliation. Ensure that you have entered your e-mail address correctly.
Please read the following instructions carefully before submitting your abstract.- All fields on the Submit Abstract form denoted by a red * are mandatory.
- To prevent submission failure, limit your abstract text to under 1,500 characters rather than the 1,520 character limit indicated.
- Use the optional Collaboration name field if required.
Please use the format: ABC Collaboration. - Use the optional Funding source field if you are obliged to do so.
- Use the Presentation type pull-down to indicate whether your abstract should be considered for Oral or Poster presentation.
If you do not indicate the presentation type, it will be considered to be a Poster. - If this abstract is for a Plenary Talk that you have been asked to present, please indicate the fact in the Comments field at the foot of the form.
- Under Track classification select the most appropriate of the twelve topics (tracks) listed below.
- Use the Submit Abstract link to the left to begin entering your abstract.
CIPANP 2018 Topics (Tracks):
Physics at High Energies- Higgs physics
- Collider searches for SUSY and other beyond-the-Standard-Model (BSM) physics
- Theoretical interpretations
- Next generation colliders – Future Circular Collider, International Linear Collider, …
- Models of BSM physics
- Muon Physics
- g-2
- muon-to-electron conversion and other lepton flavor violation
- muon capture
- muonium studies
- muonic Lamb shift
- Rare meson decays
- Weak charges of the electron and proton
- Antihydrogen
- Family and lepton number tests at high energies
- Proton decay, n-nbar oscillations
- Cosmic microwave background and its polarization
- Other high-precision cosmology
- Large-scale structure formation
- Cosmological parameters
- Re-ionization epoch
- Cosmologically generated gravitational waves
- Short-range tests of gravity and new interactions
- Astrophysical tests of general relativity
- Inflation and baryogenesis
- Theories of dark energy/inflation
- Multi-verses, cyclic universes, arrow of time
- Neutrino oscillations in neutrino beams and with reactor fluxes
- Double beta decay
- Solar and atmospheric neutrinos
- Direct neutrino mass measurements
- Cosmological constraints on neutrino mass
- Neutrino flavor physics of supernovae
- Neutrino cross section measurements
- CKM tests in neutron and nuclear beta decay
- Hadronic parity violation
- EDMs of the electron, neutron, atoms, and molecules
- P- and T-odd neutron and nuclear beta decay correlations
- Neutron lifetime
- Direct detection of WIMP dark matter
- Astrophysical searches for dark matter
- Collider searches for dark matter
- Axions and other light dark matter candidates
- Theories of dark matter and its interactions
- Instrumentation
- Supernovae: Observations and modeling
- Neutron stars and neutron star mergers
- Multi-messenger astrophysics
- Big bang nucleosynthesis
- Explosive nucleosynthesis
- Detection of high energy cosmic rays (IceCube, Pierre Auger, …)
- Cosmic ray sources and acceleration mechanisms: nucleons, nuclei, electrons/positrons, gammas, neutrinos
- Underground laboratories
- Decays, mixings, lifetimes, and CP asymmetries of charmed and b-flavored hadrons
- QCD calculations that aid in the determination of the CKM matrix
- Interpretations of non-standard model effects and extensions
- BES3, CLEO, BaBar and Belle results
- LHC flavor physics results
- Rare decays
- Lattice QCD calculations of heavy quark physics
- BSM contributions to flavor physics
- Diagonal and transition form factors
- Proton charge radius
- Light quark meson and baryon spectroscopy
- Spectroscopy of heavy quark states
- Models
- Lattice QCD calculations
- Determining hadronic properties from experimental data
- Unpolarized parton distribution functions
- Longitudinal and transverse spin structure of the nucleon
- Generalized parton distributions
- Nucleon spin
- Quark-gluon correlations
- Non-perturbative models
- Lattice QCD calculations
- Hadronization
- Polarizabilities
- Structure functions and the Coulomb sum rule
- EMC effect, color transparency
- Short-range correlations
- Nuclear forces, chiral interactions
- Nuclear models vs. ab initio methods
- Nuclei and nuclear forces from lattice QCD
- Nuclei far from the valley of stability
- Neutron-rich nuclei, nuclear matter, and the equation of state
- Nucleon and nuclear structure for fundamental symmetries
- QCD phase diagram
- Initial state effects
- Correlations and fluctuations
- Theromodynamics and hadron chemistry
- Relations to other strongly interacting systems
- Open heavy flavor and quarkonia
- Jets
