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From Understanding BasicFrom Understanding Basic
Particle Physics to exploring theParticle Physics to exploring the
UniverseUniverse
Dr. Nickolas Solomey
Professor of Physics
Wichita State University
Presented at Galaxy Forum of Kansas Cosmosphere July 27, 2013
In the last six months there have
been some great discoveries to
answer the most perplexing
questions of the Universe:
● Dark Matter and Dark Energy
● Galactic and Inter-galactic neutrinos
● Gamma Ray Bursts
● Cosmic Rays
Dark Matter and Dark Energy
● The evidence for the existence of Dark Matter
has been around for many years:
– Rotation Curves of Galaxies
– Einstein Lensing
– Universe Accelerating its expansion
● What is the Dark Matter?
and Dark Energy?
Galaxy Forum Kansas 2013 - Nick Solomey
Galaxy Forum Kansas 2013 - Nick Solomey
Galaxy Forum Kansas 2013 - Nick Solomey
Galaxy Forum Kansas 2013 - Nick Solomey
Galaxy Forum Kansas 2013 - Nick Solomey
Galaxy Forum Kansas 2013 - Nick Solomey
Galaxy Forum Kansas 2013 - Nick Solomey
Meaning of results suggest that the energies of these positrons
might have been created when particles of dark matter collided
and destroyed each other.
Neutrino Observatory
● Neutrino are an elementary particle that:
– almost never interacts with matter
– can travel through light years of lead
– can penetrate further back in time than light
● First lets explore what are neutrinos and their
rule in elementary particle physics.
● Then how neutrinos are used as an
observatory.
Galaxy Forum Kansas 2013 - Nick Solomey
Neutrino Physics
Basic Neutrino production method are nuclear
beta decay from:
– Radioactive elements decays, such as
● Nuclear Reactors
● Solar fusion reactions
● Geothermal processes in the core of the Earth
● Astronomical sources
– High energy particle physics interactions some of which
can emulate the method particles where produced in the
big bang
– Decay in flight of very heavy particles, maybe some that
are yet undiscovered
Neutrino Physics
Origins of Neutrinos
Galaxy Forum Kansas 2013 - Nick Solomey
Map of significances obtained in the IceCube-40 search for neutrino sources
(Abbasi et al., 2010a). The heavy black line indicates the Galactic plane. Note that
although the statistical variation is similar, the sensitivity and energy range probed
vary considerably between the two hemispheres.
Two very large energy neutrino events above 1 TeV have been seen and these raise
special questions such as could they come from some very massive super-particle
yet to be discovered by modern science, or are they inter-galactic neutrinos?
Skymap in equatorial coordinates of the measured probability of clustering among
the 28 events. The most significant cluster consists of five events—all showers
and including the second highest energy event in the sample.
Gamma Ray Bursts
● High Energy bursts of photons much larger in
energy than light have been seen for many
years and have been a mystery.
● New Observations with ground based and
NASA satellites have resulted in some new
ideas and understanding of these mysterious
events.
● An ultra strange event occurred last year and in
early 2013 is now understood to be a giant
class of new type of star.
Gamma Ray Bursts
● Fermi Gamma Ray Observatory
● Swift ESO Gamma Ray Observatory
Galaxy Forum Kansas 2013 - Nick Solomey
Galaxy Forum Kansas 2013 - Nick Solomey
Galaxy Forum Kansas 2013 - Nick Solomey
Cosmic Rays
● Cosmic Rays are charged particles from outside
of the earth and our solar system.
● They have a large extent of energy from a few
keV to 1019
eV.
● They still remain a mystery:
– Where do they come from
– How do they get their large energy
● But they can also be a scientific tool for study:
– Astronomy with Cosmic Ray looking for sources
– Are higher energy charged particles than man will ever
be able to make in the lab, and we can use it to study
particle physics.
Cosmic Rays
Galaxy Forum Kansas 2013 - Nick Solomey
Galaxy Forum Kansas 2013 - Nick Solomey
Future Northern Cosmic Ray experiment needs to be 100 square miles, high
altitude plateau and in a remote unpopulated area but have sufficient infrastructure.
The Kansas, Colorado, Oklahoma, New Mexico and Texas panhandle is ideal for
this.
NMNM
Conclusion
● I hope you found some of this new astro-particle
physics exciting.
● You are welcome to come to Lamar and see our
test-array, just drive 20 min. south of Lamar, CO
on high 287 and the first tank will be in the field
on the left just before reaching the big AT&T
tower.
● The next large cosmic ray experiment will be
even more exciting, but without everyone
support it may not occur due to limited research
funds.

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Galaxy Forum Kansas 2013 - Nick Solomey

  • 1. From Understanding BasicFrom Understanding Basic Particle Physics to exploring theParticle Physics to exploring the UniverseUniverse Dr. Nickolas Solomey Professor of Physics Wichita State University Presented at Galaxy Forum of Kansas Cosmosphere July 27, 2013
  • 2. In the last six months there have been some great discoveries to answer the most perplexing questions of the Universe: ● Dark Matter and Dark Energy ● Galactic and Inter-galactic neutrinos ● Gamma Ray Bursts ● Cosmic Rays
  • 3. Dark Matter and Dark Energy ● The evidence for the existence of Dark Matter has been around for many years: – Rotation Curves of Galaxies – Einstein Lensing – Universe Accelerating its expansion ● What is the Dark Matter? and Dark Energy?
  • 11. Meaning of results suggest that the energies of these positrons might have been created when particles of dark matter collided and destroyed each other.
  • 12. Neutrino Observatory ● Neutrino are an elementary particle that: – almost never interacts with matter – can travel through light years of lead – can penetrate further back in time than light ● First lets explore what are neutrinos and their rule in elementary particle physics. ● Then how neutrinos are used as an observatory.
  • 14. Neutrino Physics Basic Neutrino production method are nuclear beta decay from: – Radioactive elements decays, such as ● Nuclear Reactors ● Solar fusion reactions ● Geothermal processes in the core of the Earth ● Astronomical sources – High energy particle physics interactions some of which can emulate the method particles where produced in the big bang – Decay in flight of very heavy particles, maybe some that are yet undiscovered
  • 17. Map of significances obtained in the IceCube-40 search for neutrino sources (Abbasi et al., 2010a). The heavy black line indicates the Galactic plane. Note that although the statistical variation is similar, the sensitivity and energy range probed vary considerably between the two hemispheres.
  • 18. Two very large energy neutrino events above 1 TeV have been seen and these raise special questions such as could they come from some very massive super-particle yet to be discovered by modern science, or are they inter-galactic neutrinos?
  • 19. Skymap in equatorial coordinates of the measured probability of clustering among the 28 events. The most significant cluster consists of five events—all showers and including the second highest energy event in the sample.
  • 20. Gamma Ray Bursts ● High Energy bursts of photons much larger in energy than light have been seen for many years and have been a mystery. ● New Observations with ground based and NASA satellites have resulted in some new ideas and understanding of these mysterious events. ● An ultra strange event occurred last year and in early 2013 is now understood to be a giant class of new type of star.
  • 21. Gamma Ray Bursts ● Fermi Gamma Ray Observatory ● Swift ESO Gamma Ray Observatory
  • 25. Cosmic Rays ● Cosmic Rays are charged particles from outside of the earth and our solar system. ● They have a large extent of energy from a few keV to 1019 eV. ● They still remain a mystery: – Where do they come from – How do they get their large energy ● But they can also be a scientific tool for study: – Astronomy with Cosmic Ray looking for sources – Are higher energy charged particles than man will ever be able to make in the lab, and we can use it to study particle physics.
  • 29. Future Northern Cosmic Ray experiment needs to be 100 square miles, high altitude plateau and in a remote unpopulated area but have sufficient infrastructure. The Kansas, Colorado, Oklahoma, New Mexico and Texas panhandle is ideal for this. NMNM
  • 30. Conclusion ● I hope you found some of this new astro-particle physics exciting. ● You are welcome to come to Lamar and see our test-array, just drive 20 min. south of Lamar, CO on high 287 and the first tank will be in the field on the left just before reaching the big AT&T tower. ● The next large cosmic ray experiment will be even more exciting, but without everyone support it may not occur due to limited research funds.