Contact
information:
Email: jlj@lanl.gov
Telephone: 505-665-8739
Find me
on Linkedin
and ResearchGate
In
April 2012 our work on
the critical
metallicity for
planet
formation was reviewed
in Astrobiology
magazine. It was
also recently featured
in a LANL
news release.
In May 2012 I will be presenting our work on the formation of supermassive
stars and black holes at the First
Stars IV
conference in
Kyoto, Japan.
Our group at LANL is currently planning a workshop on the first
black holes for spring 2013. Details can be found here soon.
In January 2012 I
presented our
research on
supermassive star
formation at the 219th
AAS meeting in
Austin, TX.
I am contributing
a chapter on the
theory of the
formation of the first
galaxies to an
upcoming book in the
Springer/Astrophysics
and Space Science
Library series. A
preprint of the
chapter is available
here.
In June 2011 I participated in the First Galaxies
workshop organized by our research group at the Max
Planck Institute for
Extraterrestrial
Physics (MPE). See all of the
participants here.
In July 2010 I
presented our work on
early black holes at
the workshop What
drives the growth of
black holes?
at Durham
University in England.
In March 2010 I
presented at the
The First Stars and
Galaxies
conference at the University
of Texas at
Austin. See my
contribution to the
proceedings, Observational
Signatures of the
First Galaxies,
here.
Since the fall of 2009 I have been collaborating with other
members of the Theoretical
Modeling of Cosmic
Structures group
at MPE to study
the effects of
radiation emitted by
the first generations
of stars in the First
Billion Years
project.
In May 2009 I completed my Ph.D. in Astronomy at UT
Austin, where I
was a member of the
new Texas
Cosmology Center.
In August 2008 our simulation of radiation from the first stars
appeared in the New
York Times.
In December 2007 our work on Population III star formation in the assembly of the first galaxies was reported by the New Scientist.
Selected Recent
Research
Click on the
images at left to
read more on each
topic in a
scientific journal article.
Stellar Radiation in The First Billion Years
(coming soon)
In the First Billion Years (FiBY)
project, we have performed some of the most
sophisticated and complete cosmological simulations
of the earliest epochs of galaxy formation. We have
found that the radiation emitted from both
primordial and metal-enriched stars alters the
chemical evolution of the early universe in rich and
complex ways.
The First Planets
The first planets formed only when a sufficient amount of dust
was generated in the interstellar medium by the
first generations of stars. The first Earth-like planets
probably formed only once the abundance of heavy elements reached 10 percent
of that in our Sun. The growing collection of observational data
so far support the prevailing theory of planet formation at low metallicity.
The Stellar Seeds of Supermassive
Black Holes
The most massive stars ever
formed may have collapsed to become the
protogalactic seeds of supermassive black
holes. While the radiation they emit limits
the growth of some of these stars, the most
massive grow until they collapse. Click here to watch
a movie showing the formation of, and
accretion of primordial gas onto,
a black hole formed from a supermassive star.
The Contribution of Supernovae to Reionization
Stars are usually discussed as the
source of the photons that reionized the
Universe. Supernovae may also be
responsible for a substantial fraction of
reionization, due to the hard spectrum of
the radiation they emit. This is especially
true
for very powerful supernovae, which may have been more
common during the epoch of reionization than
they are today.