|
University Students
GCWA Student Development Office
Summer
School in Gravitational Wave Astronomy
Grid
Summer Workshop
Society of Physics Students
High School Students
Monday Night Physics
21st Century Astronomy Ambassadors Program
ARCC Student Group
Middle School Students
Physics Circus
All Ages
Science Wall
Field Trips
Past Efforts
Brownsville Alliance for
Science Education ENLACE
World Year of Physics 2005
UTBRG Relativity
Outreach Programs
GriPhyN/iVDGL Education
and Outreach Center
|
|
In honor of the
UTB/TSC
anniversary year, the Physics and Astronomy department has started a
special lecture series called, Monday Night Physics. A
seminar presented a the level of high school juniors and seniors is held the third Monday of each month.
Although high school students are encouraged to attend, all are welcome. The series is free, open
to the public, and no reservations are required. Simply come, enjoy the
talk and learn about the exciting world of Physics! All lectures are
held in the Science Engineering and Technology Building (SETB) 3rd Floor
Conference room at 7:00pm.
Campus Map
2006-2007
Schedule
|
18-Sep-06 |
Dr. Mario Diaz |
From
Einstein to Colliding Black Holes: A short history of the search
for gravitational waves |
 |
This talk gives a historical
perspective of the evolution of Einstein's
theory and the different experiments that since the late 60’s
have tried to detect gravitational waves. I'll explain why the
search is so difficult and what is different now. |
|
16-Oct-06 |
Dr. Soma
Mukherjee |
Search for Gravitational Waves in our Universe |
 |
Existence of gravitational
waves has been predicted over a hundred years ago, but so far,
there has not been a direct detection. Efforts are underway all
over the world to detect these ripples in space-time that are
expected to open a new window to our universe. The talk will
outline a description of these experiments and techniques for
searching the astrophysical sources. |
|
20-Nov-06 |
Dr.
Willem van Straten |
Radio
Pulsars and Gravitational Waves |
 |
In addition to the
gravitational wave detectors built here on Earth, such as LIGO,
or proposed to be built in orbit with Earth, such as LISA,
nature provides its own gravitational wave observatory: the test
masses are the Earth and an array of pulsars distributed around
our Galaxy, and the laser is replaced by the powerful beams of
radio emitted by each pulsar. This talk will begin with an
overview of radio pulsars, how they are observed, how they have
been used to test theories of gravity, and how they provided the
first evidence for the existence of gravitational waves. I will
then discuss the international effort to detect gravitational
waves using pulsars and some of the main challenges that lie
ahead. |
|
22-Jan-07 |
Dr. Natalia Guevara |
How Big is Nano |
 |
Nanotechnology helps scientists to build and characterize
structures and devices that are comparable in size to single
molecules. It
is expected to lead to the creation of strongest and
lightest materials, smallest and highly efficient sensors,
fastest elements in electronic devices, and, ultimately,
bring solutions to long standing problems across all
disciplines of science.
|
|
19-Feb-07 |
Dr.
Soumya Mohanty |
Transients in the sky |
 |
The night sky appears static, old
and predictable. Nothing could be further from the truth! We
will explore the domain of transient events in the sky, some of
which are the most powerful explosions of energy one can
imagine. |
|
16-Apr-07 |
Dr. Joe
Romano |
LISA:
Detecting Gravitational Waves from Space |
 |
The Laser
Interferometer Space Antenna (LISA) is a proposed joint NASA-ESA
mission whose goal is to detect low frequency (1e-4 to 1e-1 Hz)
gravitational waves. Expected sources include short period
binary stars in our galaxy, extra-galactic massive black holes,
and the capture of stellar mass objects by these black holes. In
this talk, I will briefly describe the LISA mission and the
science that LISA will be able to do with its observations. |
|
21-May-07 |
Dr.
Phillip Dukes |
The
new order for the Solar System, a 3-D tour |
 |
On 24 August 2006 the International Astronomical
Union issued a resolution redefining what a planet is. According
to this new definition, Pluto is no longer to be regarded as a
planet but now as a dwarf planet. The IAU also specified that
the largest asteroid, Ceres, and that the recently discovered
Kuiper belt object, 2003 UB313, now call Eris, are also dwarf
planets. Come learn about this new order for the Solar System
and lots more as we take a 3-D visual tour through the solar
system and beyond. |
Monday Night
Physics
is presented by
The
Department of Physics and Astronomy
Center for Gravitational Wave Astronomy
&
Brownsville Alliance for Science Education ENLACE project
Organizing Committee:
Adrienne
Rodriguez-Zermeno
Adrienne.Zermeno@utb.edu
(956) 882-6684
Robert Stone
Martha Casquette
Laura Ramirez
|
|