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2020 Fiscal Year Research-status Report

Interstellar Turbulence by Supermassive Black-Hole Jets, Winds, and Radiation

Research Project

Project/Area Number 19K03862
Research InstitutionUniversity of Tsukuba

Principal Investigator

Wagner Alexander  筑波大学, 計算科学研究センター, 助教 (20634463)

Project Period (FY) 2019-04-01 – 2022-03-31
Keywordsturbulence / star formation / hydrodynamics / galaxy formation
Outline of Annual Research Achievements

This year has seen substantial progress in this project, especially in the following tasks outlined in the original project proposal: 1) development of a fast Poisson solver capable of solving for the potential for a self-gravitating galactic disc for any box size and any boundary conditions in 3D; 2) The extension of the Poisson solver to conduct Helmholtz decompositions of the velocity field in galactic discs; 3) a completely renewed analysis of the star-formation rate in high-resolution 3D simulations of AGN jets interacting with a gas-rich galactic disc, showing, surprisingly, that positive feedback, as found in earlier work including by other groups, was incorrect. Instead, star-formation is reduced due to the strong turbulence generated by the AGN jets. Interestingly, the star-formation efficiency (the amount of stars formed per unit mass of gas) is enhanced by the same mechanism. These results have never before been seen in simulation of AGN feedback. We have partially identified a physical cause for the "negative" feedback. 4) Further analysis through the Helmholtz decomposition technique have revealed that the gas dynamics responsible for the observed change in star-formation and star-formation efficiency is due to vortical motions generated by the jet plasma flows. We are preparing two papers in which these findings will be presented. Two further papers have been submitted on turbulence-regulated AGN feedback: one exploring cloud destruction, and one showing the phenomena in ALMA observations of a radio galaxy with a massive gas disc (J2345-0449).

Current Status of Research Progress
Current Status of Research Progress

3: Progress in research has been slightly delayed.

Reason

This project relies on strong collaborations with international colleagues. While the collaborations have been ongoing, exchange of ideas and progress on individual tasks has been delayed due to the inability to visit collaborators institutes and work on problems together - a major strategy in the original proposal, for which substantial travel funds were allocated.

Another Covid-19 related reason for a slight delay was the increased burden of teaching online (including exams) and on-demand (preparing lecture videos) which reduced the time available for research by up to approximately 20%.

Occasionally, raising a 2 and 4 year old child have reduced my ability to continuously work on this project, resulting in an approximately 10% reduction in productivity.

Strategy for Future Research Activity

The next big steps in this project to be pursued in the final year are: 1) Perform full 3D magnetohydrodynamic simulations of relativistic jets interacting with gas rich galactic discs. Magnetohydrodynamic turbulence is fundamentally different to hydrodynamic turbulence, and the full analysis of how the star-formation rate and star-formation efficiencies vary with jet interaction will be performed on the new simulations; 2) Complete the physical theory of how vortical motions generated by the jets affect the star-formation rate and efficiency; 3) Perform cloud-crushing simulations of layers of turbulent radiative clouds and assess their survival rate; 4) Complete a physical picture of the negative feedback seen in the radio spiral galaxy J2345-0449.

Causes of Carryover

The Covid-19 pandemic has forced me to cancel planned collaboration visits to Australia and Paris. A laptop purchase was planned, but has been delayed to mid 2021 as the model sought has not yet been released by the maker (Apple). A new laptop will be purchased this year to replace an old one that is reaching the end of its life to continue day to day work on the project. The rest of the amount will be used to attend conferences and, if Covid-19 restrictions permit, travel to visit collaborators. If funds remain, data storage units will be purchased to store the large amounts of data generated by the new simulations and the analyses thereof.

  • Research Products

    (12 results)

All 2020 Other

All Int'l Joint Research (6 results) Journal Article (3 results) (of which Int'l Joint Research: 3 results,  Peer Reviewed: 3 results) Presentation (1 results) (of which Int'l Joint Research: 1 results) Remarks (2 results)

  • [Int'l Joint Research] The Australian National University/University of Sydney(オーストラリア)

    • Country Name
      AUSTRALIA
    • Counterpart Institution
      The Australian National University/University of Sydney
  • [Int'l Joint Research] Institut d'Astrophysique de Paris/Observatoire de la Cote d'Azur(フランス)

    • Country Name
      FRANCE
    • Counterpart Institution
      Institut d'Astrophysique de Paris/Observatoire de la Cote d'Azur
  • [Int'l Joint Research] ASTRON(オランダ)

    • Country Name
      NETHERLANDS
    • Counterpart Institution
      ASTRON
  • [Int'l Joint Research] IUCAA(インド)

    • Country Name
      INDIA
    • Counterpart Institution
      IUCAA
  • [Int'l Joint Research] Johns Hopkins University/University of Toledo/University of Northern Carolina(米国)

    • Country Name
      U.S.A.
    • Counterpart Institution
      Johns Hopkins University/University of Toledo/University of Northern Carolina
    • # of Other Institutions
      2
  • [Int'l Joint Research]

    • # of Other Countries
      5
  • [Journal Article] Gas, dust, and star formation in the positive AGN feedback candidate 4C 41.17 at z = 3.82020

    • Author(s)
      Nesvadba N. P. H.、Bicknell G. V.、Mukherjee D.、Wagner A. Y.
    • Journal Title

      Astronomy & Astrophysics

      Volume: 639 Pages: L13~L13

    • DOI

      10.1051/0004-6361/202038269

    • Peer Reviewed / Int'l Joint Research
  • [Journal Article] Shock-multicloud interactions in galactic outflows ? I. Cloud layers with lognormal density distributions2020

    • Author(s)
      Banda-Barragan W E、Bruggen M、Federrath C、Wagner A Y、Scannapieco E、Cottle J
    • Journal Title

      Monthly Notices of the Royal Astronomical Society

      Volume: 499 Pages: 2173~2195

    • DOI

      10.1093/mnras/staa2904

    • Peer Reviewed / Int'l Joint Research
  • [Journal Article] Unravelling the enigmatic ISM conditions in Minkowski’s object2020

    • Author(s)
      Zovaro Henry R M、Sharp Robert、Nesvadba Nicole P H、Kewley Lisa、Sutherland Ralph、Taylor Philip、Groves Brent、Wagner Alexander Y、Mukherjee Dipanjan、Bicknell Geoffrey V
    • Journal Title

      Monthly Notices of the Royal Astronomical Society

      Volume: 499 Pages: 4940~4960

    • DOI

      10.1093/mnras/staa3121

    • Peer Reviewed / Int'l Joint Research
  • [Presentation] Tracing the Vestigial Milky Way Jet2020

    • Author(s)
      Cecil Gerald N, Wagner Alexander Y, Bland-Hawthorn J
    • Organizer
      43rd COSPAR Scientific Assembly
    • Int'l Joint Research
  • [Remarks] Research on AGN Feedback

    • URL

      https://www2.ccs.tsukuba.ac.jp/Astro/Members/ayw/research/research.html

  • [Remarks] pyFC A fractal cube construction module

    • URL

      https://www2.ccs.tsukuba.ac.jp/Astro/Members/ayw/code/pyFC/

URL: 

Published: 2021-12-27  

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