Current Research Assistant Professor
Position Department of Physics & Institute for the Study of Earth, Oceans, and Space
245C Morse Hall, 8 College Road
University of New Hampshire
Durham, NH 03824-2600
+1(603) 862-4379
dacheng.lin@unh.edu
www.dachenglin.com
Education Massachusetts Institute of Technology (MIT) Cambridge, MA
Ph.D., Physics, September 2009 2003-2009
Thesis: The Accretion Process in the Neutron-Star Low-mass X-ray Binaries
University of Science and Technology of China (USTC) Hefei, China
B.S., Geophysics, July 2003 1998-2003
Thesis: Angular Momentum of Non-axisymmetric Steady Solar Wind
University of Science and Technology of China Hefei, China
Secondary B.E., Engineering Science, July 2002 2000-2002
Thesis: Digital Signal Processor
Awards MIT Leadership Appreciation Award (2009)
MIT Avery Ashdown Leadership Award (2008)
Winner of the American Mathematical Contest in Modeling (MCM, 2002)
Outstanding Student Scholarship (1st, 2002)
Outstanding Student Scholarship (2nd, 2001)
Outstanding Student Scholarship (1st, 2000)
Outstanding Student Scholarship (1st, 1999)
Press <1>
Black
Hole Meal Sets Record for Length and Size
(2017)
Release
Research University of New Hampshire, Department of Physics
Experience & Institute for the Study of Earth, Oceans, and Space Durham, NH
Research Assistant Professor August 2017present
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- Study
accretion process around black holes across mass scale: from
stellar-mass black holes in X-ray binaries to supermassive black
holes in galactic nuclei
- Search
for tidal disruption events (tidal disruption of stars
by otherwise dormant supermassive black holes)
- Search
for intermediate-mass black holes of mass 100--100,000 solar mass
- Study
large surveys/catalogs
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University
of New Hampshire
Institute
for the Study of Earth, Oceans, and Space
Durham, NH
Research
Scientist
February 2014-August
2017
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Investigate
the outbursting supermassive black holes at the center of galaxies,
especially their tidal disruption of stars
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Search
for distant off-nuclear intermediate-massive black holes so as to
identify the remnants of massive population III stars in the early
Universe or tidal stripping of merging satellite dwarf galaxies
containing nuclear black holes
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Study
the properties of X-ray binaries in NGC 3115 using the Chandra
extremely deep observations of this galaxy
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Study
the X-ray counterparts to Fermi unidentified GeV sources
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Improve
the unified model for neutron star low-mass X-ray binaries
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University
of Alabama, Department of Physics & Astronom Tuscaloosa,
AL
Postdoctoral
Associate
Advisor:
Prof. Jimmy A. Irwin August 2012-January 2014
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- Investigate
the outbursting supermassive black holes at the center of galaxies,
especially their tidal disruption of stars
- Search
for distant off-nuclear intermediate-massive black holes so as to
identify the remnants of massive population III stars in the early
Universe or tidal stripping of merging satellite dwarf galaxies
containing nuclear black holes
- Study
the properties of X-ray binaries in NGC 3115 using the Chandra
extremely deep observations of this galaxy.
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Institut de Recherche en Astrophysique et Planétologie Toulouse, France
Postdoctoral Associate
Advisors: Dr. Didier Barret, Dr. Natalie Webb September 2009-July 2012
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-
XMM-Newton
data screener, screening the real-time XMM-Newton data product and
producing the quality report
- Member
of XMM-Newton Science Analysis Software Developing Working Group,
including daily compiling and testing of the software
- Systematic
classification of point sources in the XMM-Newton X-ray
Serendipitous Source Catalogue, studying the long-term and
short-term X-ray variability for different classes, correlating with
other wavelengths, optimizing the criteria to differentiate
different classes, and searching for new interesting X-ray sources
with significant scientific values, such as cooling neutron stars
and new X-ray transients.
- Studying
X-ray binaries using XMM-Newton data in combinations with other
X-ray instruments.
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MIT, Department of Physics Cambridge, MA
Advisor: Dr. Ronald A. Remillard September 2003-September 2009
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Investigate
the accretion process in the neutron-star low-mass X-ray binaries
using data from many X-ray instruments, including RXTE, Chandra,
XMM-Newton, Suzaku, Swift and BeppoSAX.
- Scrutinize
RXTE/ASM weekly all-sky maps to detect new X-ray transients.
- Develop
a new solution to the decades-old problem of spectral modeling of
the accreting neutron stars.
- Analyze
the transient neutron-star binary XTE J1701-462 to find the direct
global relation among different types of accreting neutron stars and
the causes of the spectral evolution at high accretion rates.
- Develop
software for the Fourier frequency resolved spectroscopy.
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USTC, School of Earth and Space Sciences Hefei, China
Advisor: Prof. Youqiu Hu September 2002-July 2003
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-
Work
on two-fluid non-axisymmetric MHD numerical simulation of the solar
wind evolving from the sun to the earth.
- Quantify
the angular momentum in the solar wind and investigated how it transports
in the non-axisymmetric case.
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USTC, School of Earth and Space Sciences Hefei, China
Advisor: Prof. Xiankang Dou September 2001-July 2003
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- Construct
a neural-network model for space weather prediction.
- Design
neural-network software to predict the long-term space weather.
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