GRB Temporal Analysis (GTA) Workshop: Welcome & Overview
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1 GRB Temporal Analysis (GTA) Workshop: Welcome & Overview Mike Stamatikos Center for Cosmology and Astro-Particle Physics OSU Physics Research Building (PRB 4138) Columbus, OH USA June 28-30, 2010
2 Welcome to Columbus!
3 GTA Workshop: Logistics Workshop website talk repository (USB Memory Stick): Please see Lisa Krehnovi for registration materials, e.g. name tag, wireless internet instructions, updated agenda, etc. Daily Coffee Breaks & Lunches will be in lobby area outside PRB Workshop Dinner will be on Tuesday (06/29/10) at Bistro Need to get a head count for Wednesday (06/30/10). Need to get a head count for Tuesday (06/29/10).
4 GRB Temporal Analysis Consortium (GTAC) 1. Narayan Bhat (UAH) 2. Chuck Dermer (NRL) 3. Kalvir Dhuga (GW) 4. Chris Fryer (LANL) 5. Jon Hakkila (COFC) * 6. Glen MacLachlan (GW) 7. Raffaella Margutti (INAF-OAB) 8. Kohta Murase (OSU) ** 9. Jay Norris (U Denver) * 10. Brad Peterson (OSU) 11. Taka Sakamoto (NASA-GSFC) * 12. Jeff Scargle (NASA-AMES) * 13. Mike Stamatikos (OSU/NASA-GSFC) 14. Todd Thompson (OSU) 15. Kenji Toma (PSU) * 16. Tilan Ukwatta (GW) Tentative * Not able to participate in this workshop. ** Will join in on Wednesday (06/30/10).
5 GTAC: Vision & Mission Statement To form a team of theorists and experimentalists that will strategically focus on the temporal analysis of light curves from GRBs. To build a new methodological paradigm in the determination of temporal observables and explore their theoretical implications. To determine courses of action to help guide new: 1. theoretical investigations, 2. development of analysis techniques, and 3. plans for future satellite missions.
6 GTA Workshop: Major Themes Major GRB temporal analysis topics will include: 1. intrinsic variability timescale (via wavelets, FFT, etc.) 2. spectral lag (via pulse-fit paradigm, CCF, etc.) These observables in principle can be directly extracted from GRB data and may shed light upon currently untenable aspects such as: 1. the progenitor(s), 2. central engine, 3. Bulk Lorentz Factor ( Bulk ) 4. short/long class discrimination. 5. Empirical redshift estimates
7 GTA Workshop: Key Goals Various methodologies will be compared/contrasted to: 1. define the state of the art, 2. facilitate the identification of fundamental open questions associated with the temporal characteristics of GRBs, and assign key task to 3. draft a collaborative white paper outlining a unified paradigm for the determination of variability and lags, with possible implications for the minimum Bulk Lorentz factor, short/long class discrimination and progenitor/central engine models.
8 After four decades of observations, several open questions still remain...
9 Open Questions #1: Variability Timescale What is the best way to define t v? Is there an inconsistency between t v of BATSE GRBs and those from Swift/Fermi? Does t v evolve with time? Are there variability classes amongst GRBs? Since flares are a form of late time variability, what are their temporal properties? Are they time dependent? Does their total energy correlate with other observables from prompt emission such as duration, E iso, etc.? What aspects of GRB phenomenology can be tied to the central engine? Is t v correlated with the intrinsic microphysics? Can t v be used to discriminate between progenitor models?
10 Open Questions #2: Bulk Lorentz Factor In conjunction with the observed high-energy -ray emission from Fermi, t v effects the calculation of Bulk. What are the implications of Bulk~1000 for leptonic/hadronic models? Does Bulk evolve with time throughout emission? How does time-averaged Bulk correlate with E iso, E tot, X-ray plateau duration, or total energy in flares?
11 Open Questions #3: Spectral Lags What is the physical source of the spectral lag? Is there something we can learn about the central engine or is the lag a mechanism of the emission of radiation? Which is the best method to measure the spectral lag? Does spectral lag change throughout prompt emission? What is the physical explanation behind the lag-luminosity relation (LLR)? What are the implications of the presence of a LLR both in x- ray flares and in the prompt -ray pulses? Is there an intrinsic difference between the spectral lags of long and short GRBs or is it a selection effect?
12 GTA Workshop: Scientific Program This will be a "think tank" environment, with ~20+10 minute talks on Day 1 that will set the stage for open discussion, strategy & break-out sessions on Days 2-3. The agenda will be flexible and allow for extended Q&A sessions in the context of presentations. Time won t be kept in the traditional sense, but we don t want to give out any Fidel Castro Awards either! Therefore, the scientific agenda should be considered a guide rather than a strict schedule.
13 GTA Workshop: Scientific Program DAY 01: Monday (June 28, 2010) PRB :30-8:45 AM Shuttle transport from University Plaza Hotel to Physics Research Building (PRB) 8:45-9:00 AM Coffee and Registration Lisa Krehnovi 9:00-9:30 AM Welcome & Overview Mike Stamatikos 9:30-10:00 AM Variability in Gamma-Ray Sources: Bulk Lorentz Factors, Beaming Factors, and Energetics Chuck Dermer 10:00-10:30 AM Environments around Collapsar and DNS GRBs Chris Fryer 10:30 11:00 AM Coffee Break 11:00-11:30 AM Overview of Magnetars Todd Thompson 11:30-12:00 PM Some Temporal and spectral studies of a few strong GBM GRB light curves Narayan Bhat 12:00 12:30 PM BAT Spectral Lags: Average, Time resolved & The Lag-Luminosity Relation Mike Stamatikos 12:30 2:00 PM Lunch 2:00 2:30 PM Measuring Time Delays in Reverberation Studies of Active Galactic Nuclei Brad Peterson 2:30 3:00 PM Timing in the time domain Raffaella Margutti 3:00 3:30 PM A New Frequency-Luminosity Relation for Long GRBs Tilan Ukwatta 3:30-4:00 PM Coffee Break 4:00 4:30 PM A Wavelet Based Estimation of the Hurst Exponent from Long GRBs Glen MacLachlan 4:30-5:30 PM Strategy Session: Identifying Open Questions All 5:30-5:45 PM Shuttle transport from Physics Research Building (PRB) to University Plaza Hotel
14 GTA Workshop: Scientific Program DAY 02: Tuesday (June 29, 2010) PRB :30-8:45 AM Shuttle transport from University Plaza Hotel to Physics Research Building (PRB) 8:45-9:00 AM Coffee and Registration Lisa Krehnovi 9:00-9:30 AM Summary of Day 01 Mike Stamatikos 9:30-10:30 AM Strategy Session: Developing Working Groups & Action Items All 10:30 11:00 AM Coffee Break 11:00 12:30 PM Breakout Session: Theory & Experiment Working Groups 12:30 2:00 PM Lunch 2:00 3:30 PM Breakout Session: Theory & Experiment Working Groups 3:30-4:00 PM Coffee Break 4:00-5:15 PM Working Group Summary: Plan for Future Work All 5:30-7:30 PM Workshop Dinner (Bistro 2110) 7:30-7:45 PM Shuttle transport from Physics Research Building (PRB) to University Plaza Hotel Need to get a head count.
15 GTA Workshop: Scientific Program DAY 03: Wednesday (June 30, 2010) PRB :30-8:45 AM Shuttle transport from University Plaza Hotel to Physics Research Building (PRB) 8:45-9:00 AM Coffee and Registration Lisa Krehnovi 9:00-9:30 AM Summary of Day 02 Mike Stamatikos 9:30-10:30 AM Strategy Session: Outline for White Paper All 10:30 11:00 AM Coffee Break 11:00 11:45 PM Strategy Session: Future Analysis Tasks and Action Items All 11:45-12:00 PM Closing Remarks: End of Workshop Mike Stamatikos 12:00 PM Lunch Make sure to check out and bring luggage with you to OSU. We can facilitate scheduling taxi service to CMH. Need to get a head count.
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