Colloquia & Seminars

Colloquia & Seminars

Department of Physics & Astronomy Colloquia and Seminars Series

2026 - 2027 Program

Virtual or R-150, Hilbun Hall, Mississippi State University

Fridays @ 3:00 PM

NB: Unless noted otherwise, Physics Colloquia/Seminars are held as mentioned above

 

  • September 11th, 2026  Dr. Chao-Chin Yang, Department of Physics & Astronomy, University of Alabama

    Title: From pebbles to planets: planetesimal formation and pebble accretion

    Host: Dr. Lamiaa El Fassi

    Instruction: In-person in Hilbun R-150

    Abstract: Despite the thousands of extrasolar planetary systems already detected, indicating the ubiquity of planets around stars, a comprehensive picture of how planets are formed from their natal protoplanetary disks remains to be drawn.  From interstellar μm-sized dust grains to newborn planets, planet formation covers 30 orders of magnitude in mass and 13 orders of magnitude in size.  Moreover, planet formation involves complicated interactions between the solid materials, the gaseous medium, the stellar irradiation, and the magnetic fields.

                   I will review our current understanding of the dust-gas dynamics in protoplanetary disks and its consequences on the formation of planets via the core accretion scenario.  Specifically, I will examine how and under what conditions cm/mm-sized dust pebbles can actively concentrate themselves to high density for km-sized planetesimals to form, the initial mass function of planetesimals, and how pebble accretion assists planet formation, along with some supporting observational evidence.

     

  • September 18th, 2026  Dr. Xiaochun He, Physics and Astronomy Department, Georgia State University

      Titile: gLOWCOST Comes to Mississippi State: Cosmic Rays as a Global Sensor for Space and Terrestrial Weather

      Host: Dr. Wenliang (Bill) Li

      Instruction: In-person in Hilbun R-150

      Abstract: Secondary cosmic rays reaching the ground carry an imprint of everything they have passed through — solar activity and heliospheric conditions, the geomagnetic field, and the state of the atmosphere itself. A single detector records this as a fluctuating count rate. A distributed network of detectors, sampling many locations continuously, turns those fluctuations into a measurement.
                  gLOWCOST is a growing collaboration built around exactly this idea: compact, inexpensive muon detector nodes, each built on a Raspberry Pi platform with custom front-end electronics, deployed at universities and schools and streaming time-stamped count rates to a central server. Because the hardware is affordable and reproducible, the network can scale in a way that traditional instrumentation cannot, and because students build, install, and maintain the nodes, each site is also a training environment.
                  In this talk I will describe the scientific case for the network — sensitivity to solar transients and heliospheric modulation on one hand, and to atmospheric pressure, temperature, and severe weather on the other — and what a dense, geographically distributed array makes possible that isolated instruments do not. I will present the current status of the network, recent results from deployed nodes, and measurements taken beyond the ground: detector flights aboard commercial aircraft and a balloon flight probing the altitude dependence of the secondary flux.
                 I will close with the long-term vision for gLOWCOST and with an invitation, as Mississippi State joins the collaboration, to help shape what comes next. 

 

  • September 25th, 2026  Dr. Kenny Wunder, Department of Economics, Finance, & Legal Studies, The University of Alabama

     Titile: Defining Moments: Taking Physics into the Social Sciences

      Host: Dr. Donna Pierce

      Instruction: In-person in Hilbun R-150

      Abstract: In this talk I share my experience moving from physics into the social sciences. My aim is to help you see what you have really been learning as a physics student and how that training applies well beyond the context of physics. I will discuss other career options available to you, why these alternative pathways may be worth your attention, and how you can take advantage of the skills you have already developed to set out in a direction you may not have considered. Along the way I will describe what research in the social sciences looks like and how it differs from research in the hard sciences, and I will talk about some of my own work and how it pertains directly and indirectly to my physics foundations.

 

  • October 2nd, 2026  Dr. Garth Huber, Department of Physics, University of Regina

      Titile: TBD

      Host: Dr. Wenliang (Bill) Li

      Instruction: In-person in Hilbun R-150

      Abstract: 

 

  • October 9th, 2026  Fall Break. Be safe and enjoy :)!

 

  • October 16th, 2026  Dr. Huong Nguyen, Department of Physics, University of Virginia

    Titile: TBD

     Host: Dr. Dipangkar Dutta

     Instruction: In-person in Hilbun R-150

     Abstract: 

 

    Titile: TBD

     Host: Dr. Prabhakar Pradhan

     Instruction: In-person in Hilbun R-150

     Abstract: 

 

  • October 30th, 2026  Dr. Andre Sieverding, Space Science Institute, Lawrence Livermore National Laboratory

     Titile: TBD

     Host: Dr. Jaspreet Randhawa

     Instruction: In-person in Hilbun R-150

     Abstract: 

 

     Titile: TBD

     Host: Dr. Lamiaa El Fassi

     Instruction: In-person in Hilbun R-150

     Abstract: 

 

  • November 13th, 2026  Ms. Eva Godwin & Mr. Maruf Abubakar, Physics & Astronomy Department, Mississippi State University

    Titile: TBD

     Host: Drs. Angelle Tanner and Jaspreet Randhawa

     Instruction: In-person in Hilbun R-150

     Abstract: 

 

  • November 20th, 2026  Dr. Ryan Wang, Department of Physics and Astronomy, University of Alabama

     Titile: TBD

     Host: Dr. Lamiaa El Fassi

     Instruction: In-person in Hilbun R-150

     Abstract: 

 

  • November 27th, 2026  Thanksgiving Break. Be safe and enjoy :)!

 

  • December 1st, 2026  End of Semester. Happy Holidays :)!

 

  • Past Colloquia/Seminars 

 

  • September 4th, 2026  Dr. Emanuele Usai, Department of Physics & Astronomy, University of Alabama

Title: Building the CMS High Granularity Calorimeter for the High-Luminosity LHC

Host: Dr. Lamiaa El Fassi

Instruction: In-person in Hilbun R-150

Abstract: In June 2026 the Large Hadron Collider completed its third run and entered a long shutdown to prepare for its most ambitious phase yet: the High-Luminosity LHC (HL-LHC). From 2030, the upgraded machine will collide protons at up to ten times the LHC's design luminosity, piling 140–200 interactions into every bunch crossing (up from roughly 60 in the run just ended) on the way to a dataset of 3000 fb⁻¹, six times everything collected so far. That data will improve our understanding of the Higgs boson, the top quark, and extend the reach for new physics, but it comes at a price: radiation levels and event complexity far beyond what parts of the CMS detector were built to survive. The answer in the endcap regions, where doses will reach 2 MGy, is the High Granularity Calorimeter (HGCAL): the first large-scale silicon-based imaging calorimeter at a hadron collider, with 47 sampling layers per endcap, 620 m² of silicon sensors and six million readout channels in all, operating at −35 °C with timing precision of a few tens of picoseconds to reconstruct particle showers in position, energy, and time. HGCAL's basic unit is the silicon module, read out by a "hexaboard": a hexagonal circuit board carrying radiation-tolerant HGCROC chips wire-bonded to the sensor beneath. I will motivate the HL-LHC physics program, describe the design of HGCAL, and present our group's contribution to its ongoing construction: the electrical testing and quality control of hexaboards, where measurements of pedestals, noise, and injected-charge response decide whether each of thousands of boards is fit to spend the 2030s just meters from the highest-energy proton collisions ever produced. Finally, I will briefly describe physics measurements that will be made possible at HL-LHC.

 

  • August 28th, 2026  Dr. Zexi Xing, Department of Physics, Auburn University 

Title: Long-term volatile evolution of Interstellar comet 3I/ATLAS

Host: Dr. Angelle Tanner

Instruction: In-person in Hilbun R-150

Abstract: Interstellar comets are visitors to our Solar System from other planetary systems and provide rare macroscopic samples of material formed around other stars. Their activity should reveal the chemical inventory of extrasolar planetesimals, but cometary comae are shaped by how volatiles are stored, buried, exposed and released. Swift monitored water activity in the third known interstellar object, 3I/ATLAS, as it approached, passed, and receded from the Sun. Water production rose rapidly, remained high near perihelion, and then declined steeply. The coma changed from CO₂-rich activity far from the Sun to an H₂O-rich coma near perihelion and CO-rich activity after perihelion. The area needed to produce the observed water exceeded the surface area of the nucleus, indicating an extended source of icy grains. Its integrated mass loss corresponds to an approximately 11 m global shell for a 1.3 km nucleus, potentially excavating through a processed surface layer. Observations of 3I/ATLAS show that cometary composition changes with time as a product of volatile storage, release and erosion. This evolution must be followed when using comets to probe protoplanetary disks.

 

  • August 21st, 2026  Dr. Vaniya Ansari, Physics and Astronomy Department, Mississippi State University

    Title: Unfolding the Proton Spin Puzzle: SpinQuest at Fermilab

    Host: Dr. Lamiaa El Fassi

    Instruction: Virtual on ZOOM ONLY

      Abstract: In 1987, the European Muon Collaboration discovered that quark spins account for only a fraction of the proton's total spin. Nearly four decades later, the proton spin decomposition is still an unsolved puzzle. One key piece of that puzzle is how a quark's transverse momentum correlates with the spin of the proton carrying it — a relationship captured by transverse-momentum-dependent parton distributions, and in particular by the Sivers function. The Sivers function of sea antiquarks remains especially poorly known.

    SpinQuest (E1039), running in the fixed-target beamlines at Fermilab, is built to close that gap. It measures transverse single-spin asymmetries in polarized Drell-Yan scattering: a 120 GeV unpolarized proton beam striking a transversely polarized ammonia (NH₃) or deuterated-ammonia (ND₃) target. At forward rapidity, Drell-Yan production is uniquely sensitive to the antiquark content of the polarized target — giving a clean, direct handle on the antiquark Sivers function that semi-inclusive DIS can't offer, since quark and antiquark contributions are tangled together there.

   Extracting that signal is an apparatus challenge as much as a physics one. Sustaining high, stable polarization under highbeam intensity requires a cryogenic target held near 1 Kelvin in a 5 Tesla field, with radiation damage continuously repaired through target annealing. This talk covers the physics motivation behind SpinQuest, the experimental setup — especially the polarized target system — and first-stage results on the transverse single-spin asymmetry in J/ψ production.
 

 

Click here for 2025 - 2026 season

 

2026-2027 Committee

Anatoli Afanasjev (325-2918, aa242-at-msstate.edu email)
Lamiaa El Fassi (Chair) (325-0627, le334-at-msstate.edu email)
Seong-Gon Kim (325-8031, sk162-at-msstate.edu email)
Donna Pierce (325-2914, dmp149-at-msstate.edu email)                                                          Prabhakar Pradhan (325-6626, pp838-at-msstate.edu email)
Jaspreet Randhawa (325-2688, jsr512-at-msstate.edu email)
Chuji Wang (325-9455, cw175-at-msstate.edu email)
Secretary: Tracy Wilcox (325-2159, tld25-at-msstate.edu email)