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Archive for the ‘Seminars’ Category


NPP Seminar by Joseph Atchison (ACU)

March 10th, 2022 by geurts

Date: Tuesday May 3, 2022 at 4pm
Location: HBH 227 + online

Title: The Electric Conductivity of Hot Pion Matter
Speaker: Joseph Atchison (ACU)

Abstract

The determination of transport coefficients plays a central role in characterizing hot and dense nuclear matter. Currently, there are significant discrepancies between various calculations of the electric conductivity of hot hadronic matter. It has been shown that dilepton emission spectra can be described by calculating the electromagnetic correlator within the vector dominance model (VDM). Transport coefficients probe the low-energy limit of the medium, thus the interactions of the low mass pion are expected to play an important role in determining the conductivity of hot hadronic matter. In the present work we calculate the electric conductivity of hot pion matter by extracting it from the electromagnetic spectral function, as its zero energy limit at vanishing 3-momentum. Within the VDM the photon couples primarily to the rho meson. Therefore, we use hadronic many-body theory to calculate the rho meson’s self-energy in hot pion matter. This requires the dressing of the pion propagators within the rho self-energy with thermal π-ρ and π- σ loops, and the inclusion of vertex corrections to maintain gauge invariance. In particular, we analyze the transport peak of the spectral function and extract its behavior with temperature.

NPP Seminar by Dorian Praia-Do-Amaral (Durham University, IPPP)

March 1st, 2022 by geurts

Date: Tuesday March  1, 2022 at 4pm
Location: online

Title: Discovering New Neutrino Physics at Dark Matter Direct Detection Experiments with Solar Neutrinos
Speaker: Dorian Praia-Do-Amaral (Durham University, IPPP)

Abstract

The next generation of dark matter direct detection experiments will become so sensitive that they will begin to expose themselves to an irreducible background of solar neutrinos, complicating the search for dark matter. However, this will also present them with the compelling opportunity to search for neutrino physics beyond the Standard Model. In this talk, I will show how direct detection experiments will be able to use solar neutrinos as invaluable messengers of potential light new physics in the neutrino sector.

I will begin with a short introduction to the gauged $U(1)_{L_\mu – L_\tau}$ model—an elegant possible extension to the Standard Model. This model introduces a new gauge boson that couples to neutrinos and can stand to not only resolve the observed tension in the muon’s anomalous magnetic moment, but also rectify the long-standing discrepancy between early- and late-time measurements of the Hubble constant. I will show that, by treating the solar neutrino rate as a signal, direct detection experiments will be sensitive to as-yet unprobed regions of this model’s parameter space able to explain both of these anomalies simultaneously. Furthermore, I will argue that, with some enhancements to its projected experimental configuration, the far-future experiment DARWIN will be able to make a 5$\sigma$ discovery of this new gauge boson.

These findings indicate that direct detection experiments will become key players in the search for new neutrino physics, providing us with entirely new information on physics beyond the Standard Model.

NPP Seminar by Lauren Yates (Fermilab)

February 22nd, 2022 by geurts

Date: Tuesday February  22, 2022 at 4pm
Location: HBH 227 + online

Title: Recent Results from MicroBooNE Addressing the MiniBooNE Anomaly
Speaker: Lauren Yates (Fermilab)

Abstract

The MicroBooNE experiment uses a liquid argon time projection chamber (LArTPC) located on-axis in the Booster Neutrino Beam at Fermilab to perform a wide variety of physics measurements. Recently, MicroBooNE released its first results addressing the nature of the anomalous excess of low-energy interactions previously observed by the MiniBooNE collaboration. This seminar will focus on an approach that isolates electron neutrino interactions consistent with the kinematics of charged-current quasi-elastic (CCQE) events. The topology of such signal events has a final state with one electron and one proton (1e1p). Multiple novel techniques are employed to identify a 1e1p final state, including particle identification that uses two methods of deep-learning-based LArTPC image analysis and event selection using a boosted decision-tree ensemble trained to recognize two-body scattering kinematics.

NPP Seminar by Austin Baty (Rice University)

February 1st, 2022 by geurts

Date: Tuesday Feb. 1, 2022 at 4pm
Location: HBH 227 + online

Title: TRILLION DEGREE MATTER: Probing the Emergence of the Quark-Gluon Plasma
Speaker: Austin Baty (Rice University)

Abstract

Using high-energy nucleus-nucleus collisions, physicists are able to study the trillion-degree soup of quarks and gluons that existed in the very early universe. This strongly-interacting matter, known as the quark-gluon plasma, exhibits unique properties including the suppression of high-momentum particle production and behavior as a ‘nearly-perfect’ fluid. Surprisingly, some of these signals have also been observed in smaller systems, such as proton-proton collisions, prompting questions about the minimum conditions needed to observe such phenomena. I will describe my experimental efforts to clarify this issue using recent lead-lead collision data from the CMS detector at the LHC, as well as archived data from previous particle colliders. In addition, I will discuss exciting opportunities for the future at both the LHC and RHIC, which will usher in a new era of understanding regarding strongly interacting matter.

NPP Seminar by Peter Gaemers (NIKHEF)

January 24th, 2022 by geurts

Date: Tuesday Jan. 25, 2022 at 4pm
Location: HBH 227 + online

Title: Xenon Analysis
Speaker: Peter Gaemers (NIKHEF)

Abstract

The XENON collaboration has developed the liquid xenon time-projection chamber technology into the leading technology for searching for WIMP dark matter. The recent upgrade of XENON1T has completed and resulted in the XENONnT experiment. I briefly introduce the working principle of liquid xenon time-projection chamber before diving into details about how the data acquisition system works. This is the system responsible for the readout of the signals coming for the time-projection chamber. The focus of the talk will be teaching students about the required steps to go from PMT signals to processed data ready for analysis, and how they were designed.

NPP Seminar by Corey James (ANL)

November 2nd, 2021 by geurts

Date: Tuesday Nov. 2, 2021 at 4pm
Location: online

Title: Machine Learning and Deep Learning in the NEXT Neutrinoless Double Beta Decay Experiment
Speaker: Corey James (ANL)

Abstract

In the search for experimental observation of neutrinoless double beta decay, the Neutrino Experiment with a Xenon TPC (NEXT) program seeks to leverage both state of the art energy resolution as well as high resolution topological discrimination to separate double beta decay candidates from radiogenic and other backgrounds. In this talk, I will describe the NEXT Program and highlight it’s use of artificial intelligence and machine learning techniques to search for neutrinoless double beta decay.

NPP Seminar by Melissa Quinnan (UCSB)

October 15th, 2021 by geurts

Date: Tuesday Oct. 19, 2021 at 4pm
Location: online

Title: Standard Model Four-Top Production with the CMS Detector (Run II)
Speaker: Melissa Quinnan (UCSB)

Abstract

Standard model four top quark production is a rare process with great potential to reveal new physics. Measurement of the cross section is not only a direct probe of the top quark Yukawa coupling with the Higgs, but an enhancement of this cross section is predicted by several beyond the standard model (BSM) theories. This process is studied in fully-hadronic proton-proton collision events collected during Run II of the CERN LHC by the CMS detector, which corresponded to an integrated luminosity of 137fb−1 and a center of mass energy of 13TeV. In order to optimize signal sensitivity with respect to significant and challenging backgrounds, several novel machine-learning based tools are applied in a multi-step and data-driven approach. Boosted decision tree (BDT) and deep neural net (DNN) based hadronic top taggers are used to identify hadronically decaying top quark candidates with moderate and high transverse momenta, respectively, in order to suppress backgrounds and categorize events by the multiplicity of reconstructed top tags, and an event-level kinematic BDT distribution is subsequently used to extract the signal. Control regions inspired by the “ABCD” method are used to obtain a data-driven estimate of the background, and data distributions in these control regions are given as inputs to a DNN in order to estimate the event-level BDT discriminant distributions of the major backgrounds. In combination with searches in other decay modes the expected significance of this analysis is estimated to reach at least 3 standard deviations, corresponding to the “evidence” of standard model four top production.

NPP Seminar by Chris Tunnell (Rice)

August 27th, 2021 by al72

Date: Tuesday Aug 31, 2021 at 4pm
Location: HBH 227

Title: The bizzare excess electronic recoil events in XENON1T
Speaker: Chris Tunnell (Rice)

Abstract

XENON1T is the most sensitive dark matter detector built to date, but its senstivity has opened up a range of other scientific searches and discoveries. I will tell the story of one such search and the evidence we have for solar axions, a neutrino magnetic moment, or tritium. This result gained substaintial interest in the field with nearly 300 citations in the last year. I will also explain why each explaination is slightly unsettling, where XENONnT (our upgrade) should help clarify this situation.

NPP Seminar by Isaac Upsal (BNL)

April 27th, 2021 by geurts

Date: Tuesday April  27, 2021 at 4pm
Location: online

Title: Exploring the Frontier of Vorticity in Heavy-ion Collisions
Speaker: Isaac Upsal (BNL)

Abstract

In accelerators like RHIC, heavy atomic nuclei are collided at high energies to study emergent properties of the strong-nuclear force. At high-enough energies with heavy-enough nuclei such collisions create a short-lived novel fluid of deconfined quarks and gluons called the “Quark Gluon Plasma”. Because the nuclei themselves are so large, the transverse size of the nuclear overlap is a variable of significance to the field. Collisions with large impact parameters (low degree of overlap) have large angular momentum (~1000 hbar). For a collision which takes a finite amount of time one would expect an excess of particles with spin along the direction of system angular momentum due to spin-orbit coupling.

In 2017 STAR reported the first non-trivial measurement of this alignment, called the global polarization, at the order of a few percent (https://doi.org/10.1038/nature23004). In a thermalized fluid this polarization would come about through a vorticity. Using such a framework it’s possible to extract a vorticity on the order of 10^22 s^-1, which is notably higher than any previously known fluid. This measurement renewed interest in this physics within the heavy-ion physics community and there have been a number of interesting new calculations as well as measurements from STAR, ALICE, and HADES. I plan on discussing this measurement, newer developments, and the future of similar measurements.

NPP Seminar by Taylor Faucett (UCI)

January 25th, 2021 by geurts

Date: Wednesday January  27, 2021 at 2pm
Location: online (YouTube)

Title: Physicists Learning from Machines Learning
Speaker: Taylor Faucett (UCI)

Abstract

Machine Learning methods are extremely powerful but often function as black-box problem solvers, providing improved performance at the expense of clarity. Our work describes a new machine learning approach which translates the strategy of a deep neural network into simple functions that are meaningful and intelligible to the physicist, without sacrificing performance improvements. We apply this approach to benchmark high-energy problems of fat-jet classification and electron identification. In each case, we find simple new observables which provide additional classification power and novel insights into the nature of the problem.