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TCAN-MBH | The multi-scale physics of massive black holes

The multi-scale physics of massive black holes. The discovery that supermassive black holes (SMBHs) with masses greater than 10. Solar masses are in place within a billion years after the Big Bang represents a formidable theoretical challenge for current models of structure formation in the early Universe. How are such behemoths assembled in such a short time? The answer to this fundamental question relies on the solution to yet another unsolved problem:. Georgia Institute for Technology.

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TCAN-MBH | The multi-scale physics of massive black holes | tcan.gatech.edu Reviews

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The multi-scale physics of massive black holes. The discovery that supermassive black holes (SMBHs) with masses greater than 10. Solar masses are in place within a billion years after the Big Bang represents a formidable theoretical challenge for current models of structure formation in the early Universe. How are such behemoths assembled in such a short time? The answer to this fundamental question relies on the solution to yet another unsolved problem:. Georgia Institute for Technology.

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TCAN-MBH | The multi-scale physics of massive black holes | tcan.gatech.edu Reviews

https://tcan.gatech.edu

The multi-scale physics of massive black holes. The discovery that supermassive black holes (SMBHs) with masses greater than 10. Solar masses are in place within a billion years after the Big Bang represents a formidable theoretical challenge for current models of structure formation in the early Universe. How are such behemoths assembled in such a short time? The answer to this fundamental question relies on the solution to yet another unsolved problem:. Georgia Institute for Technology.

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2015 Atlanta Meeting | TCAN-MBH

http://www.tcan.gatech.edu/2015-atlanta-meeting

The multi-scale physics of massive black holes. Our first collaboration meeting will be held on March 3-4, 2015 at the Georgia Institute of Technology, located in Midtown Atlanta. We will meet in the CRA Visualization Lab (room 1-90) in the Boggs Building. See this map. For directions, shuttle stops, visitor parking lots, nearby subway stops, and selected nearby hotels. There will be a $35 registration fee to cover break refreshments and supplies. Please pay the fee in this link. Tuesday, March 3rd.

2

Network | TCAN-MBH

http://www.tcan.gatech.edu/network

The multi-scale physics of massive black holes. Georgia Institute of Technology. Our project is partitioned into the 3 crucial stages that need to be understood about the lives of massive black holes:. The formation of the first black hole seeds. The physics of the fueling of growing black holes. The energetics of the feedback that SMBHs exert on their environment. 2015-16 TCAN Webinar Series. Upcoming TCAN Postdoc Seminars. TCAN Seminar on AGN Fueling. Inaugural TCAN Webinar (Formation of SMBHs).

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Publications | TCAN-MBH

http://www.tcan.gatech.edu/publications

The multi-scale physics of massive black holes. Publications from this TCAN. Smith, B., Glover, S., Natarajan, P. N. Khochfar, S. 2015, “New constraints on direct collapse black hole formation in the early Universe”,. Johnson, J. L., Zackrisson, E., Labbe, I., van den Bosch, F. C., Natarajan, P. Khochfar, S. 2015, “Detecting Direct Collapse Black Holes: making the case for CR7”,. H-Y K Yang, C. S. Reynolds. SA Balbus, A.Schekochohin. D Lazzati, B. J. Morsony. Journal of High Energy Astrophysics. K Park, ...

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2015-16 TCAN Webinar Series | TCAN-MBH

http://www.tcan.gatech.edu/news/2015-16-tcan-webinar-series

The multi-scale physics of massive black holes. 2015-16 TCAN Webinar Series. We have just kicked off our second TCAN webinar series for this academic year. It will be held once or twice a month with four talks scheduled before the new year. The talks are generally on Friday at 11am Eastern. Here is planned schedule,. October 30th) Chris Reynolds, University of Maryland: “The (inefficient) driving of bulk turbulence by active galactic nuclei in the intracluster medium” ( slides. Leave a Reply Cancel reply.

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Upcoming TCAN Postdoc Seminars | TCAN-MBH

http://www.tcan.gatech.edu/news/upcoming-tcan-postdoc-seminars

The multi-scale physics of massive black holes. Upcoming TCAN Postdoc Seminars. In preparation for our annual TCAN meeting in March, we have scheduled the TCAN Postdocs to give seminars on their research. If you’re at one of the network nodes, feel free to attend the seminar, as it’s open to everyone. We will post the slides here after each talk. The seminars will be held on the following Tuesdays at 11am and will consist of a 40 minute talk, followed by a 40 minute discussion period.

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Members | Computational Cosmology at Georgia Tech

http://cosmo.gatech.edu/members

Computational Cosmology at Georgia Tech. The first stars: formation and feedback. Dwarf galaxy formation and evolution. Black hole growth in the early universe. Group in Aug 2015. L-R: Shi, Koh, Barrow, Gilbert, Aykutalp, Wise, Cunningham, Nelson, Ge. Inset: Park. Group in Aug 2015. L-R: Wise, Shi, Barrow, Aykutalp, Ge, Gilbert, Koh, Cunningham, Nelson. Inset: Park. Photos taken by postdoc Claudia Lazarro on her last day at the CRA! Postdoc; primary mentor: Bogdanovic. Kevin Choi (Physics / CS). Erin Cal...

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Aycin Aykutalp | Computational Cosmology at Georgia Tech

http://cosmo.gatech.edu/members/aycin-aykutalp

Computational Cosmology at Georgia Tech. The first stars: formation and feedback. Dwarf galaxy formation and evolution. Black hole growth in the early universe. Postdoctoral Researcher ( TCAN. PhD in Astrophysics, University of Groningen (2012). BSc in Physics, University of Ankara. Publication list from ADS. Van Kempen, T. A. 24 authors (including A. Aykutalp. 2015, “Outflow forces in intermediate mass star formation”,. 797, 139 ( arXiv. Mesinger, A., Aykutalp, A. 8221;, MNRAS, submitted ( arXiv.

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TCAN-MBH | The multi-scale physics of massive black holes

The multi-scale physics of massive black holes. The discovery that supermassive black holes (SMBHs) with masses greater than 10. Solar masses are in place within a billion years after the Big Bang represents a formidable theoretical challenge for current models of structure formation in the early Universe. How are such behemoths assembled in such a short time? The answer to this fundamental question relies on the solution to yet another unsolved problem:. Georgia Institute for Technology.

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