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DTSTART:19450814T190000
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BEGIN:VEVENT

CATEGORIES:Natural Sciences
CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=8a0292fd-8d13410f-018d-cc5e605b-00004257:Angelica M
 itchell\, J.D.
CREATED:20250811T153405Z
DESCRIPTION:The upcoming Legacy Survey of Space and Time (LSST) will deliv
 er larger catalogs of solar system object orbits\, sizes\, colors\, and l
 ight curves than any survey to date. However\, all surveys are subject to
  observational and algorithmic bias\, skewing their catalogs' distributio
 ns away from the intrinsic. To prepare to characterize LSST's survey bias
 es\, we develop methods and tools to quantify the selection function of a
  wide-field solar system survey as a function of all six orbital paramete
 rs and absolute magnitude. We apply these methods to debias a novel Helio
 LinC3D search for Centaurs in the Pan-STARRS1 detection catalog\, confirm
 ing a literature Centaur model's marginal distributions\, rejecting its j
 oint distribution\, and estimating an intrinsic population of 21\,400 Cen
 taurs with Hr < 13.7. We use Sorcha\, a new solar system survey simulator
 \, to simulate the ten-year LSST detection catalog of a full-scale solar 
 system\, including cutting-edge population models of near-Earth objects\,
  main belt asteroids\, Jupiter Trojan\, and trans-Neptunian objects. This
  catalog offers the best predictions of the LSST solar system yield and i
 s made publicly available\, allowing researchers to test new methods\, al
 gorithms\, and software on LSST-like data before the survey is conducted.
  Future work includes applying these methods to LSST.
DURATION:PT1H
DTSTAMP:20250811T153405Z
DTSTART;TZID=America/New_York:20250828T140000
LAST-MODIFIED:20250811T153405Z
LOCATION;X-BEDEWORK-UID=18832edc-1c2ecfef-011c-32333fc8-00000043:Physics 2
 98
STATUS:CONFIRMED
SUMMARY:Cosmology Seminar- Debiasing the Solar System with LSST
UID:CAL-8a00ec8b-979413b9-0198-99c47649-000050e8demobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Natural Sciences:/user/publi
 c-user/Topics/Natural Sciences
X-BEDEWORK-SPEAKER:Jake Kurlander
X-BEDEWORK-DUKE-SERIES:Cosmology Seminar Series
X-BEDEWORK-SUBMITTEDBY:amm342 for Physics (agrp__ArtsandSciences_Physics)
END:VEVENT
BEGIN:VEVENT

CATEGORIES:Natural Sciences
CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=8a0292fd-8d13410f-018d-cc5e605b-00004257:Angelica M
 itchell\, J.D.
CREATED:20250801T150111Z
DESCRIPTION:Active Galactic Nuclei (AGN) feedback plays an important role 
 in galaxy formation\, impacting star formation and gas conditions across 
 a range of physical and temporal scales. Without AGN feedback\, modern co
 smological simulations fail to replicate global galaxy properties. Howeve
 r\, each simulation employs a unique prescription that can vary dramatica
 lly in its treatment of the underlying physical mechanisms. One promising
  means of better constraining these AGN feedback models is through the ci
 rcumgalactic medium\, as CGM gas should be impacted in differing ways bas
 ed on the implementation of feedback in each simulation. In this talk\, I
  will explore how the AGN feedback prescriptions in the SIMBA and EAGLE s
 imulations shape the CGM. I will assess the observability of these differ
 ences by generating mock thermal Sunyaev-Zel'dovich and X-ray observation
 s and comparing against stacked CGM observations from the Atacama Cosmolo
 gy Telescope and the eROSITA-SRG instrument. I will also present work mod
 ifying the AGN treatment in the SIMBA simulation\, directly probing the i
 mpact different modes of feedback can have on AGN host galaxies and the C
 GM. These results will help determine how current and upcoming missions c
 an be used to constrain models of AGN feedback in cosmological simulation
 s.
DURATION:PT1H
DTSTAMP:20250801T150111Z
DTSTART;TZID=America/New_York:20250911T140000
LAST-MODIFIED:20250801T150111Z
LOCATION;X-BEDEWORK-UID=18832edc-1c2ecfef-011c-32333fc8-00000043:Physics 2
 98
STATUS:CONFIRMED
SUMMARY:Cosmology  Seminar- Simulating the Impact of AGN Feedback on X-ray
  and tSZ Observations
UID:CAL-8a00ec8b-979413b9-0198-6626bbe7-0000359ademobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Natural Sciences:/user/publi
 c-user/Topics/Natural Sciences
X-BEDEWORK-SPEAKER:Skylar Grayson
X-BEDEWORK-DUKE-SERIES:Cosmology Seminar Series
X-BEDEWORK-SUBMITTEDBY:amm342 for Physics (agrp__ArtsandSciences_Physics)
END:VEVENT
BEGIN:VEVENT

CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Research
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=00f1fcdb-0f068baf-010f-068baf83-00000004:None
CREATED:20250806T161435Z
DESCRIPTION:A variety of low-energy\, high-precision experiments\, such as
  atomic spectroscopy and lepton scattering\, are used to test the electro
 weak structure of light nuclei. The theory support for these experiments 
 is often rooted in modern effective field theory (EFT) techniques. Howeve
 r\, it is necessary to include the effects of radiative corrections at th
 e precision relevant for many experiments\, which comes with new challeng
 es that have previously been unaddressed in the nuclear EFT paradigm. In 
 this talk\, we outline a consistent treatment of radiative corrections in
  pionless EFT using the velocity renormalization group originally develop
 ed in the context of nonrelativistic quantum chromodynamics. We present r
 enormalization group improved calculations of the deuteron charge form fa
 ctor and radiative capture process\, which are relevant for charge radius
  extractions and Big Bang nucleosynthesis\, respectively.
DURATION:PT1H
DTSTAMP:20250812T162458Z
DTSTART;TZID=America/New_York:20250916T153000
LAST-MODIFIED:20250812T162458Z
LOCATION;X-BEDEWORK-UID=18832edc-1c2ecfef-011c-32333fc8-00000043:Physics 2
 98
STATUS:CONFIRMED
SUMMARY:Triangle Nuclear Theory Colloquium - Radiative corrections and the
  renormalization group in few-nucleon systems
UID:CAL-8a00ec8b-979413b9-0198-8029bb2e-000000fbdemobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Research:/user/public-user/T
 opics/Research
X-BEDEWORK-STUDENT-CONTACT;X-BEDEWORK-PARAM-EMAIL=roxanne.springer@duke.ed
 u:Roxanne Springer
X-BEDEWORK-SPEAKER:Thomas Richardson
X-BEDEWORK-DUKE-SERIES:Triangle Nuclear Theory Colloquium
X-BEDEWORK-LOCATION:Physics Room 298
X-BEDEWORK-SUBMITTEDBY:lac135 for Physics (agrp__ArtsandSciences_Physics)
END:VEVENT
BEGIN:VEVENT

CATEGORIES:Natural Sciences
CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=8a0292fd-8d13410f-018d-cc5e605b-00004257:Angelica M
 itchell\, J.D.
CREATED:20251014T140957Z
DESCRIPTION:Using DESI DR2 baryon acoustic oscillation distance measuremen
 ts and Planck cosmic microwave background distance priors\, we have measu
 red the dark energy density ρX(z) and dark energy equation of state wX(z)
  as free functions of redshift (smoothly interpolated from values at z=0\
 ,1/3\,2/3\,1\,4/3\,2.33)\, and find both to be consistent with a cosmolog
 ical constant\, with only deviations of 1.2σ for ρX(z) and 1.9σ for wX(z)
  at z=2/3. Our results differ noticeably from those of the DESI Collabora
 tion\, in which they used the same DESI DR2 data combined with Planck dat
 a and found a 3.1σ deviation from a cosmological constant\, a finding whi
 ch is the consequence of their assuming the parametrization wX(z)=w0+wa(1
 −a). Our results indicate that assuming a linear wX(z) could be misleadin
 g and precludes discovering how dark energy actually varies with time at 
 higher redshifts. In our quest to discover the physical nature of dark en
 ergy\, the most urgent goal at present is to determine definitively wheth
 er dark energy density varies with time. We have demonstrated that it is 
 of critical importance to measure dark energy density as a free function 
 of redshift from data. I will discuss our results\, and the important rol
 es for space missions Roman and Euclid in advancing our understanding of 
 dark energy.
DURATION:PT1H
DTSTAMP:20251014T140957Z
DTSTART;TZID=America/New_York:20251106T140000
LAST-MODIFIED:20251014T140957Z
LOCATION;X-BEDEWORK-UID=18832edc-1c2ecfef-011c-32333fc8-00000043:Physics 2
 98
STATUS:CONFIRMED
SUMMARY:Cosmology Seminar- Model-Independent Dark Energy Measurements from
  DESI DR2 Data
UID:CAL-8a00ec8b-979413b9-0199-e30e6f0c-0000135bdemobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Natural Sciences:/user/publi
 c-user/Topics/Natural Sciences
X-BEDEWORK-SPEAKER:Yun Wang
X-BEDEWORK-DUKE-SERIES:Cosmology Seminar Series
X-BEDEWORK-SUBMITTEDBY:amm342 for Physics (agrp__ArtsandSciences_Physics)
END:VEVENT
BEGIN:VEVENT

CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Research
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=00f1fcdb-0f068baf-010f-068baf83-00000004:None
CREATED:20260128T223709Z
DESCRIPTION:The pressure-energy relations in the nucleon are derived from 
 the gravitational form factors\, which parameterize matrix elements of th
 e energy-momentum tensor (EMT)\, together with EMT conservation. The stat
 ic pressure distribution arising from the Lorentz trace part of the EMT\,
  as manifested in the spatial stress $\\frac{1}{3} T^{ii}$\, equals minus
  the corresponding trace part of the energy density\, which can be unders
 tood in terms of the gluon and quark condensates.  It can be shown that t
 his trace-anomaly- and sigma-term-induced pressure plays a fundamental ro
 le in the confinement dynamics of QCD. In contrast\, the dynamic pressure
  distribution from the traceless part of the spatial stress tensor equals
  $1/d$ of the corresponding traceless part of the energy density\, where 
 $d$ is the spatial dimension. We point out that the same pressure-energy 
 relations also hold for vortices in type-II superconductors\, where the s
 tatic pressure-energy relation originates from the Cooper-pair condensate
 . Furthermore\, identical equations of motion appear in the $\\Lambda{\\r
 m CDM}$ model of cosmology\, where the static pressure-energy relation ar
 ises from the cosmological constant.
DURATION:PT1H
DTSTAMP:20260330T180921Z
DTSTART;TZID=America/New_York:20260331T153000
LAST-MODIFIED:20260330T180921Z
LOCATION;X-BEDEWORK-UID=18832edc-1c2ecfef-011c-32333fc8-00000043:Physics 2
 98
STATUS:CONFIRMED
SUMMARY:Triangle Nuclear Theory Colloquium - Pressure-Energy Equations of 
 State of Hadrons\, Superconductor Vortices\, and the Cosmos
UID:CAL-8a00eca5-9af98aae-019c-06c0df76-0000209fdemobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Research:/user/public-user/T
 opics/Research
X-BEDEWORK-STUDENT-CONTACT;X-BEDEWORK-PARAM-EMAIL=haiyan.gao@duke.edu:Haiy
 an Gao
X-BEDEWORK-SPEAKER:Keh-Fei Liu
X-BEDEWORK-DUKE-SERIES:Triangle Nuclear Theory Colloquium
X-BEDEWORK-SUBMITTEDBY:lac135 for Physics (agrp__ArtsandSciences_Physics)
END:VEVENT
BEGIN:VEVENT

CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Research
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=00f1fcdb-0f068baf-010f-068baf83-00000004:None
CREATED:20260327T233946Z
DESCRIPTION:Atomically thin character of a two-dimensional (2D) material e
 nsures that it is significantly influenced by neighbors\, thereby resulti
 ng in strong proximity effects [1]: A situation when a 2D material acquir
 es properties absent in a pristine state\, such as superconductivity\, ma
 gnetism\, topological structure or an enhanced spin-orbit coupling (SOC).
  Two-dimensional (2D) Dirac materials host the electron Dirac points with
  gapless linear dispersion close to the Fermi energy and are actively bei
 ng studied for its nontrivial behavior. In this talk I'm going to discuss
  several prominent phenomena realized in 2D Dirac systems with strong pro
 ximity effects.\nUnlike in the 3D case\, the protection of Dirac gapless 
 points in 2D is not robust [2]: In the absence of this protection\, the g
 ap opening favors topological effects induced by the generation of a fini
 te Berry curvature. In our work [3]\, we have combined this with Dirac po
 ints detached from high symmetry points of the Brillouin zone and have st
 udied topological phenomena emerging in 2D materials with movable Dirac p
 oints that can be further controlled by ferroelectrics (FEs). I will disc
 uss topology-enforced kink\nelectronic states at structural domain walls 
 separating opposite FE polarizations and also show that the position of m
 ovable Dirac points modifies the dipole character of the Berry curvature\
 , responsible for switching between the zero and nonzero secondharmonic n
 onlinear Hall conductivity. These predictions can be realized in a wide r
 ange of identified 2D materials\, which is\nsupported by first-principles
  analysis of Cl2Rh2S2-GeS junction.\nFurthermore\, a monolayer graphene\,
  the most remarkable example of a 2D material with Dirac points\, with pr
 oximity effects from either magnetic\, antiferromagnetic or heavy element
 -based materials gets an enhanced SOC\, which promotes the spin-charge in
 terconversion (SCI) [4]. I will discuss how the SCI emerging from spin-ps
 eudospin proximity terms in the Dirac Hamiltonian manifests itself for ac
 -electrical driving across different frequencies: From terahertz range\, 
 where the spin-flip absorption features strong enhancement and anomalous 
 polarization structure [5]\, to mid-infrared range\, where SOC-proximity 
 gives rise to a fine structure of cyclotron resonances\, and up to visibl
 e range where it leads to the remarkable mixing of s- and p- excitons wit
 h a strong brightening of spin-forbidden p-excitons in the absorption spe
 ctrum [6].
DURATION:PT1H
DTSTAMP:20260327T233946Z
DTSTART;TZID=America/New_York:20260402T113000
LAST-MODIFIED:20260327T233946Z
LOCATION;X-BEDEWORK-UID=18832edc-1c2ecfef-011c-32333fc8-00000043:Physics 2
 98
STATUS:CONFIRMED
SUMMARY:Condensed Matter Seminar - Proximity-induced phenomena in two-dime
 nsional Dirac materials: From topological kink states to a spin-charge in
 terconversion
UID:CAL-8a003384-9cc4d1fe-019d-31ab0b10-00001573demobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Research:/user/public-user/T
 opics/Research
X-BEDEWORK-SPEAKER:Konstantin Denisov
X-BEDEWORK-DUKE-SERIES:Condensed Matter Seminar
X-BEDEWORK-STUDENT-CONTACT;X-BEDEWORK-PARAM-EMAIL=gleb.finkelstein@duke.ed
 u:Gleb Finkelstein
X-BEDEWORK-IMAGE-X1:993
X-BEDEWORK-IMAGE-Y1:113
X-BEDEWORK-IMAGE-X2:993
X-BEDEWORK-IMAGE-Y2:113
X-BEDEWORK-IMAGE-CROP-WIDTH:0
X-BEDEWORK-IMAGE-CROP-HEIGHT:0
X-BEDEWORK-IMAGE-ALT-TEXT:Proximity-induced phenomena in two-dimensional D
 irac materials
X-BEDEWORK-SUBMITTEDBY:lac135 for Physics (agrp__ArtsandSciences_Physics)
X-BEDEWORK-IMAGE:/public/Images/medium-F1_20260327113946PM.png
X-BEDEWORK-THUMB-IMAGE:/public/Images/medium-F1_20260327113946PM-thumb.png
 
END:VEVENT
BEGIN:VEVENT

CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Research
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=00f1fcdb-0f068baf-010f-068baf83-00000004:None
CREATED:20260409T150640Z
DESCRIPTION:Because of its flat energy bands\, the two-dimensional electro
 n gas exhibits a rich set of ground states\, commonly classified in two d
 ifferent classes. Fractional quantum Hall states form one class of ground
  states\; numerous fractional states support Abelian excitations\, but th
 e most interesting ones host non-Abelian excitations. Charge ordered grou
 nd states\, such as the Wigner solid\, electronic bubbles\, and electroni
 c stripe phases form a second class of ground states. In this talk I will
  highlight the profound influence of the structure of the single-electron
  wavefunction on the formation of these two classes of ground states in t
 he twodimensional electron gas hosted in GaAs/AlGaAs quantum wells. In pa
 rticular\, I will discuss two recent experimental findings: a) the quantu
 m phase transition from a non-Abelian fractional state to a stripe phase 
 when the single-electron wavefunction has a single node and b) the prolif
 eration of bubbles for single-electron wavefunctions with a complex nodal
  structure.
DURATION:PT1H
DTSTAMP:20260409T150640Z
DTSTART;TZID=America/New_York:20260409T113000
LAST-MODIFIED:20260409T150640Z
LOCATION;X-BEDEWORK-UID=18832edc-1c2ecfef-011c-32333fc8-00000043:Physics 2
 98
STATUS:CONFIRMED
SUMMARY:Condensed Matter Seminar - Structure of the Single-Electron Wavefu
 nction and Ground States in Flat Electronic Bands
UID:CAL-8a003384-9cc4d1fe-019d-72c7f4b3-00002d92demobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Research:/user/public-user/T
 opics/Research
X-BEDEWORK-SPEAKER:Gabor Csathy
X-BEDEWORK-DUKE-SERIES:Condensed Matter Seminar
X-BEDEWORK-STUDENT-CONTACT;X-BEDEWORK-PARAM-EMAIL=gleb.finkelstein@duke.ed
 u:Gleb Finkelstein
X-BEDEWORK-SUBMITTEDBY:lac135 for Physics (agrp__ArtsandSciences_Physics)
END:VEVENT
BEGIN:VEVENT

CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Research
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=00f1fcdb-0f068baf-010f-068baf83-00000004:None
CREATED:20260407T155314Z
DESCRIPTION:Because of its flat energy bands\, the two-dimensional electro
 n gas exhibits a rich set of ground states\, commonly classified in two d
 ifferent classes. Fractional quantum Hall states form one class of ground
  states\; numerous fractional states support Abelian excitations\, but th
 e most interesting ones host non-Abelian excitations. Charge ordered grou
 nd states\, such as the Wigner solid\, electronic bubbles\, and electroni
 c stripe phases form a second class of ground states. In this talk I will
  highlight the profound influence of the structure of the single-electron
  wavefunction on the formation of these two classes of ground states in t
 he twodimensional electron gas hosted in GaAs/AlGaAs quantum wells. In pa
 rticular\, I will discuss two recent experimental findings: a) the quantu
 m phase transition from a non-Abelian fractional state to a stripe phase 
 when the single-electron wavefunction has a single node and b) the prolif
 eration of bubbles for single-electron wavefunctions with a complex nodal
  structure.
DURATION:PT1H
DTSTAMP:20260409T135914Z
DTSTART;TZID=America/New_York:20260409T113000
LAST-MODIFIED:20260409T135914Z
LOCATION;X-BEDEWORK-UID=18832edc-1c2ecfef-011c-32333fc8-00000043:Physics 2
 98
STATUS:CONFIRMED
SUMMARY:Condensed Matter Seminar - Structure of the Single-Electron Wavefu
 nction and Ground States in Flat Electronic Bands
UID:CAL-8a003384-9cc4d1fe-019d-68a5e0eb-000068a6demobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Research:/user/public-user/T
 opics/Research
X-BEDEWORK-STUDENT-CONTACT;X-BEDEWORK-PARAM-EMAIL=gleb.finkelstein@duke.ed
 u:Gleb Finkelstein
X-BEDEWORK-DUKE-SERIES:Condensed Matter Seminar
X-BEDEWORK-SUBMITTEDBY:lac135 for Physics (agrp__ArtsandSciences_Physics)
END:VEVENT
BEGIN:VEVENT

CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Research
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=00f1fcdb-0f068baf-010f-068baf83-00000004:None
CREATED:20260416T212543Z
DESCRIPTION:Description Forthcoming
DURATION:PT1H
DTSTAMP:20260416T212543Z
DTSTART;TZID=America/New_York:20260430T113000
LAST-MODIFIED:20260416T212543Z
LOCATION;X-BEDEWORK-UID=18832edc-1c2ecfef-011c-32333fc8-00000043:Physics 2
 98
STATUS:CONFIRMED
SUMMARY:Condensed Matter Seminar - Title Forthcoming
UID:CAL-8a003384-9cc4d1fe-019d-982f836a-000032bbdemobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Research:/user/public-user/T
 opics/Research
X-BEDEWORK-SPEAKER:Dali Sun
X-BEDEWORK-DUKE-SERIES:Condensed Matter Seminar
X-BEDEWORK-STUDENT-CONTACT;X-BEDEWORK-PARAM-EMAIL=divine.kumah@duke.edu:Di
 vine Kumah
X-BEDEWORK-SUBMITTEDBY:lac135 for Physics (agrp__ArtsandSciences_Physics)
END:VEVENT
BEGIN:VEVENT

CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Research
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=00f1fcdb-0f068baf-010f-068baf83-00000004:None
CREATED:20260220T222827Z
DESCRIPTION:A central goal of the future Electron-Ion Collider and of upco
 ming upgrades at the Large Hadron Collider is the search for a new regime
  of nuclear matter known as the Color Glass Condensate (CGC). In this ext
 reme state\, matter is dominated by an exceptionally dense system of gluo
 ns\, the particles responsible for binding quarks inside protons and nucl
 ei. Over the past two decades\, predictions from the CGC effective theory
  have been confronted with data from HERA\, RHIC\, and the LHC\, yielding
  intriguing hints of gluon saturation\, although definitive evidence rema
 ins elusive.\n\nIn this colloquium\, I will review recent developments in
  the CGC framework and discuss how this physics can be explored through m
 easurements at current and future colliders. I will highlight several nov
 el observables that offer promising new avenues for uncovering this dense
  gluonic regime. I will conclude with a brief discussion of the CGC's bro
 ader connections to other areas of physics.
DURATION:PT1H
DTSTAMP:20260325T164329Z
DTSTART;TZID=America/New_York:20260526T153000
LAST-MODIFIED:20260325T164329Z
LOCATION;X-BEDEWORK-UID=18832edc-1c2ecfef-011c-32333fc8-00000043:Physics 2
 98
STATUS:CONFIRMED
SUMMARY:Triangle Nuclear Theory Colloquium - Mining for gluon saturation a
 t colliders
UID:CAL-8a003294-9c52b03d-019c-7d2b2beb-00001410demobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Research:/user/public-user/T
 opics/Research
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-STUDENT-CONTACT;X-BEDEWORK-PARAM-EMAIL=bass@duke.edu:Steffen Ba
 ss
X-BEDEWORK-SPEAKER:Farid Salazar
X-BEDEWORK-DUKE-SERIES:Triangle Nuclear Theory Colloquium
X-BEDEWORK-SUBMITTEDBY:lac135 for Physics (agrp__ArtsandSciences_Physics)
END:VEVENT
END:VCALENDAR