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lab:2025-02-12 [2025/01/30 08:47]
singhj created
lab:2025-02-12 [2025/02/12 20:26] (current)
singhj
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 [[public:​Current Schedule]] [[public:​Current Schedule]]
  
-**Speaker = [[https://​www.kent.edu/​physics/​profile/​veronica-dexheimer|Prof. Veronica Dexheimer]]** of Kent State University+**Speaker = [[https://​www.kent.edu/​physics/​profile/​veronica-dexheimer|Prof. Veronica Dexheimer]]** of [[https://​www.kent.edu/​physics/​center-nuclear-research|Kent State University]]
  
 Host = Sorensen, Agnieszka [[sorensen@frib.msu.edu]] Host = Sorensen, Agnieszka [[sorensen@frib.msu.edu]]
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 <​sortable>​ <​sortable>​
 ^ Start Time ^ End Time ^ Name ^ Building ^ Room ^ ^ Start Time ^ End Time ^ Name ^ Building ^ Room ^
-| 09:00 | 09:30 |    |  +| 09:00 | 09:30 | Agnieszka Sorensen ​FRIB 2000 |  
-| 09:30 | 10:00 |    |  +| 09:30 | 10:00 | Jaideep Taggart Singh FRIB 2016 |  
-| 10:00 | 10:30 |    +| 10:00 | 10:30 | Jerome Margueron ​FRIB 2131 
-| 10:30 | 11:00 |  |  |  |  +| 10:30 | 11:00 | Filomena Nunes FRIB  ​| ​2107 |  
-| 11:00 | 11:30 |    |  +| 11:00 | 11:30 | <​del>​Scott Pratt</​del>​ BreakFRIB 2102 |  
-| 11:30 | 12:00 |    +| 11:30 | 12:00 | Bill Lynch FRIB 1010 
 | 12:00 | 13:00 | Lunch with Graduate Students | FRIB | 2311 |  | 12:00 | 13:00 | Lunch with Graduate Students | FRIB | 2311 | 
-| 13:00 | 13:30 |    |  +| 13:00 | 13:30 | Break FRIB 2102 |  
-| 13:30 | 14:00 |    +| 13:30 | 14:00 | Sudhanva Lalit FRIB 2061 
-| 14:00 | 14:30 |    |  +| 14:00 | 14:30 | Dean Lee FRIB 2103 |  
-| 14:30 | 15:00 |    +| 14:30 | 15:00 | Witold Nazarewicz ​FRIB 2059 
 | 15:00 | 15:30 | Speaker Prep time | FRIB | 1300 |  | 15:00 | 15:30 | Speaker Prep time | FRIB | 1300 | 
 | 15:30 | 16:30 | Seminar | FRIB | 1300 |  | 15:30 | 16:30 | Seminar | FRIB | 1300 | 
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 ===== Context ===== ===== Context =====
  
-Title = TBD+Title = An overview of the MUSES cyberinfrastructure and what it can do for you
  
 Abstract Abstract
 <​blockquote>​ <​blockquote>​
-TBD+At high energy, the fundamental description of matter (Quantum Chromodynamics or QCD) is currently only directly applicable to specific regimes, leaving large portions of the QCD phase diagram uncharted, especially around the regime relevant for neutron stars. To bridge different regimes, the MUSES collaboration has built a cyberinfrastructure that provides descriptions of matter based on first-principle theories and models across the multidimensional QCD phase diagram, including thermodynamics but also observables pertinent to heavy-ion collisions, astrophysics,​ and more. Our online platform allows users to choose different descriptions (with different parametrizations),​ how these are connected, and what observables they reproduce. The platform is open for everyone, and all our code is open source.
 </​blockquote>​ </​blockquote>​
  
 Relevant background with commentary from Prof. Dexheimer: Relevant background with commentary from Prof. Dexheimer:
-  * I think that this paper would be useful for the students: +  * I think that this paper would be useful for the students: [[https://​doi.org/​10.1007/​s41114-024-00049-6|Theoretical and experimental constraints for the equation of state of dense and hot matter]]. It is a long paper, but you could cover only Sections 1 and 2. I will discuss in detail Fig. 1 in my seminar. 
-[[https://​doi.org/​10.1007/​s41114-024-00049-6|Theoretical and experimental constraints for the equation of state of dense and hot matter]]. It is a long paper, but you could cover only Sections 1 and 2. I will discuss in detail Fig. 1 in my seminar.+{{ :​lab:​screenshot_2025-02-07_at_09.33.16.png?​600 |}}
lab/2025-02-12.1738244846.txt.gz · Last modified: 2025/01/30 08:47 by singhj