Radiation, Hydrodynamics, and Spectral Modeling of Indirect-Drive Fusion Experiments on the OMEGA Laser David S. Conners, Katherine L. Penrose, David H.

Slides:



Advertisements
Similar presentations
Stars! A star is a large hot ball of plasma, which generates energy in its core by nuclear fusion.
Advertisements

Grating Phase-Contrast Imaging for Diagnostic of High Energy Density Plasmas D. Stutman, M.P. Valdivia, M. Finkenthal Department of Physics & Astronomy.
Energy Consumption Fossil Fuel Contribution to Global Energy Demand Year.
Inertial Confinement Fusion Experiments & Modeling Using X-ray Absorption Spectroscopy of Thin Tracer Layers to Diagnose the Time-Dependent Properties.
By: David Sundine II & Emilio Zavala.  Is anything that has mass and takes up space.  Its unit is a Atoms  It can be changed.
Physics of Fusion Lecture 1: The basics Lecturer: A.G. Peeters.
Astronomy 1020-H Stellar Astronomy Spring_2015 Day-29.
Simulation of Hohlraum Radiation Environments and Tracer Spectra in Doped Ablator Experiments * J. J. MacFarlane Prism Computational Sciences, Madison,
Heat & Energy Transfer Reassessment Review Directions To start click “Slide Show” and “From Beginning” As you go through the PowerPoint, take DETAILED.
Creating an X-ray Nebula in the Laboratory: Spectral Diagnostics of Neon Photoionization Experiments on the Z-Machine D. S. Conners, D. H. Cohen (Swarthmore.
The Sun - Our Star Sun’s diameter 100 times the Earth’s
Nuclear Physics Year 13 Option 2006 Part 2 – Nuclear Fusion.
Can you guess why I am showing you this picture?
Copyright © 2012 Pearson Education, Inc. Radius: 6.9  10 8 m (109 times Earth) Mass: 2  kg (300,000 Earths) Luminosity: 3.8  watts Our Star.
Announcements Star Assignment 2, due Monday March 15 –READ chapter 15, do Angel quiz Global Warming Project, due Wednesday March 17 –Sample 4 web sites.
We undertook an experimental campaign to study the effects of dopants on the radiation physics of ablators in indirect- drive hohlraum environments as.
Simulations investigating the effect of a DT-ice-covered cone tip on the implosion of a re-entrant cone-guided ICF capsule J. Pasley - University of California.
HANNAH SILVER, SPENCER LUKE, PETER TING, ADAM BARRETT, TORY TILTON, GABE KARP, TIMOTHY BERWIND Controlled Nuclear Fusion.
Modeling X-Ray Photoionization Experiments Michael Rosenberg and David Cohen Swarthmore College Introduction In order to reliably determine the temperature,
Big Science at a Small College: Fusion Experiments at the World's Largest Laser David Cohen Department of Physics and Astronomy with Dave Conners (’03),
X-Ray Photoionization Experiments with Intense Z-Pinches: Creating an X-Ray Binary in the Laboratory David Cohen (Swarthmore College) with Nathan Shupe.
Fusion Technology Institute University of Wisconsin - Madison NRL IFE Concepts Project 9/19/ Output Calculations for Laser Fusion Targets ARIES Meeting.
Modeling Studies of Photoionization Experiments Driven by Z-Pinch X-rays Nathan Shupe and Professor David Cohen Department of Physics and Astronomy, Swarthmore.
Power of the Sun. Conditions at the Sun’s core are extreme –temperature is 15.6 million Kelvin –pressure is 250 billion atmospheres The Sun’s energy out.
RRP:10/17/01Aries IFE 1 Liquid Wall Chamber Dynamics Aries Electronic Workshop October 17, 2001 Robert R. Peterson Fusion Technology Institute University.
Chapter 17: Evolution of High-Mass Stars. Massive stars have more hydrogen to start with but they burn it at a prodigious rate The overall reaction is.
THE STAR OF OUR SOLAR SYSTEM Solar radiation travels from the sun to the earth at the speed of light. The speed of light is km/s.
The Life Cycle of a Star I can describe the life cycle of a star u Bell ringer – What type of magnitude is each definition referring to? 1. The true.
Comparison of Stark Broadening and Doppler Broadening of Spectral Lines in Dense Hot Plasmas By Michael Zellner.
Honors Forensic Science.  Introduction  Organic substances constitute a substantial portion of physical evidence submitted to crime labs  Carbon does.
During the nineteenth century, scientists suggested that the Earth was hundreds of millions of years old. During the nineteenth century, scientists suggested.
Chemical, Biological and Environmental Engineering A Few Comments About Fusion.
Nuclear Fusion Katharine Harrison. Why Are We Interested? There are great challenges that are associated with fusion, but there are also very large possible.
40 Nuclear Fission and Fusion After fusion, the total mass of the light nuclei formed in the fusion process is less than the total mass of the nuclei that.
Future of Antiproton Triggered Fusion Propulsion Brice Cassenti & Terry Kammash University of Connecticut & University of Michigan.
The Sun Section 26.1.
Chapter 10 Bellringer Henry David Thoreau once said, “The sun is but a morning star.” What do you think this quotation means?
Energy and Earth Energy The ability to do work and produce heat.
The Sun is a mass of Incandescent Gas A gigantic nuclear furnace.
For each atom, in its natural state, the number of electrons and the number of protons is equal. This number may or may not be the same as the number.
Jeopardy Jeopardy PHY101 Chapter 11 Review Study of Nuclear Physics Cheryl Dellai.
ENERGY TRANSFER I * Energy on our planet originates from the Sun
Fusion: Basic Principles, Current Progress and ITER Plans
The Sun Unit 6: Astronomy.
Fusion in the Stars Nunez & Panogalinog. Nuclear Fusion in stars is one of the most important reasons which make life on Earth possible! ○ HOW IS THAT.
Scott Hildreth – Chabot College – Adapted from Essential Cosmic Perspective 4 th ed. Copyright 2007 by Pearson Publishing. Chapter 10 Our Star.
Review: Evolution of Sun As usual, PowerPoint slides available at the web site Dr. Bill Pezzaglia 1.
Forms of Energy. Nature of Energy Energy is the ability to do work. If an object or organism does work, then it uses energy. Work is the use of a force.
Nuclear Chemistry. Nuclear Chemistry looks at the number of protons and neutrons in an atom Radioactive Decay = Spontaneous disintegration of a nucleus.
The Sun By: JGilliam The Sun’s CompositionIdentifying Stars Composition ▪ Hydrogen and Helium together make up 99% of the sun’s mass. ▪ 75% of the sun’s.
Our Sun.
The mass of the nuclei produced is less than the mass of the original two nuclei The mass deficit is changed into energy We can calculate the energy released.
 The sun is believed to be roughly 4.6 billion years of age.  Early scientist use to believe that the sun generated its energy by burning fuel.  This.
Off the Main Sequence - The Evolution of a Sun-like Star Stages
Main sequence Hydrogen Fusion: Inside the sun, 4 Hydrogen nuclei fuse to form 1 Helium nucleus, releasing light, heat and radiation.
It’s all about energy. Energy and its transfer controls Earth’s systems.
Please remember to sit in assigned seats… before bell rings Outcome: SWBAT Compare and contrast nuclear fusion and fission by reviewing a video and creating.
Modeling of Z-Ablation I. E. Golovkin, R. R. Peterson, D. A. Haynes University of Wisconsin-Madison G. Rochau Sandia National Laboratories Presented at.
MAGNETIC CONFINEMENT FUSION Zack Draper | Physics 485 November 23, 2015.
Fusion. Examples ● Fusion is the reaction that produces the energy in the sun.
Matter in Extreme Conditions at LCLS:
FUSION PROPULSION.
Fusion and Fission.
BUCKY Simulations of Z and RHEPP Experiments
Nuclear Fusion.
Outside the nucleus, the beta decay {image} will not occur because the neutron and electron have more total mass than the proton. This process can occur.
The Structure of the Sun
Unit 5.4 Nuclear Fission and Fusion
THE UNIVERSE Part 1: stars.
Life Cycle of a Star.
Presentation transcript:

Radiation, Hydrodynamics, and Spectral Modeling of Indirect-Drive Fusion Experiments on the OMEGA Laser David S. Conners, Katherine L. Penrose, David H. Cohen (Swarthmore College and Prism Computational Sciences) and Joseph J. MacFarlane (Prism Computational Sciences) What is Inertial Confinement Fusion? Problem: the high temperatures and densities required to overcome the Coulomb barrier and join positively charged nuclei together result in high a pressure that tends to push fusion plasma apart. Energy can be indirectly delivered to the fuel capsule by firing lasers into an enclosure called a hohlraum that contains the capsule; The hohlraum converts the laser energy into thermal X-rays. In order to generate efficient fuel compression, it is important to control and diagnose the way the X-rays in the hohlraum interact with the fuel capsule. Control: Adding dopants (like bromine or germanium) to the outer layers of the fuel capsule (the ablator) influences how the radiation field inside the hohlraum interacts with the ablator. Diagnose: The spectroscopy of NaCl tracer layers buried in the ablator can be used to measure time-dependent conditions in the ablator and thus to characterize the effects of doping on compression. Experimental Design OMEGA Experiments April 2000 Time dependent backlit K α absorption spectroscopy of the NaCl tracer. Hohlraum radiation field parameters set in model to match DANTE measurements. DANTE is an absolutely calibrates ten channel X-ray detector. Goal: To compare spectra of doped and undoped ablator samples. Fusion is the joining together of hydrogen nuclei to form a more massive nucleus, releasing large amounts of energy in the process. A hydrodynamic simulation of the ablation and compression of a solid plastic sample by thermal X- rays. X-rays are incident form the left. The fusing of Deuterium and Tritium (two isotopes of Hydrogen) into Helium. Modeling It takes three steps to create a simulated absorption spectrum for comparison with real data: 1. What is the time-dependent radiation spectrum incident on the ablator sample? 2. What is the hydrodynamic response of the ablator sample to the hohlraum radiation field? BUCKY is a one dimensional hydrodynamics code that takes the radiation field spectrum output from VISRAD and models how the ablator sample’s position, density, and temperature change during the experiment. Bucky simulation of changes over time in the density of a doped plastic ablator exposed to thermal X-rays. 3. How do the spectra generated by the tracer layer in the ablator change over time? SPECT3D is a spectral analysis program written by Joseph MacFarlane of Prism Computational Sciences that can take the hydro-dynamical output from Bucky and simulate a spectrum of the tracer in the ablator sample. Comparing the Model with Data Conclusions Simulated absorption spectrum of chlorine from a salt tracer in undoped plastic ablator. Spectrum was generated at 1000 ps using 841 atomic energy levels of chlorine. Acknowledgments We gratefully acknowledge the support of the Department of Energy through grant DE-FG03- 98DP00250, the Delaware Space Grant Consortium. We would also like to thank Eric Jensen and all the Swarthmore students in the Physics & Astronomy department for their help and support over the last two years. Conservation of momentum causes the fuel to move inward, reaching a core density 20 times that of lead. Note that the fuel is pushed inward, so its own inertia acts to impede its disassembly; hence the term inertial confinement fusion. A spherical plastic fuel capsule filled with hydrogen is bombarded with energy. One solution: The inertial confinement of plasma. This heating causes the outer layer of the plastic to ablate, meaning a rocket-like blow off of material. The thermonuclear burning starts at the core and rapidly spreads throughout the fuel- this is referred to as ignition. Time = 200ps Time = 600psTime = 1000ps VISRAD is a view-factor code written by Joseph MacFarlane of Prism Computational Sciences that allows us to model the radiation field inside the hohlraum and generate the spectrum incident on the ablator. The lasers deliver 7.5kilojoules of energy inside the hohlraum. Notice the “hotspots” where the lasers come in contact with the hohlraum. The ablator sample is the circular area on the far end of the hohlraum. Screen shot from VISRAD showing the lasers entering the hohlraum. A radiation spectrum incident on the ablator at 1000ps It is possible to measure backlit absorption spectra in a hohlraum radiation environment. Doping ablator materials results in a later tracer turn-on time of chlorine K α absorption lines, indicative of the slowing down of the radiation wave by the dopant. Overall, for both the doped and undoped ablator samples, chlorine K α absorption lines are present earlier than was predicted. h x 1s 2p 2s Beryllium-likeHelium-like h x energy We take advantage of the affinity that X- rays have for inner shell electrons. How do we learn things from looking at the chlorine absorption spectra? When the radiation shock wave arrives at the NaCl tracer layer, it provides energy for electrons to make upward transitions resulting in K absorption lines. The appearance of these lines provides us with a local time- dependent diagnostic of the X-ray interaction with the ablator sample. Energy level diagram showing electrons making K α transitions. For more information or to download this poster, please visit Bucky simulation of changes over time in the temperature of a doped plastic ablator exposed to thermal X-rays. undoped plastic1.5% germanium dopant Changes over time in absorption spectra generated by tracer layers in the actual undoped and doped plastic ablators used in the April 2000 experiments. Note the delay in the appearance of K α absorption signals on the undoped and doped sides. Comparison of actual and simulated absorption spectra of salt tracer in undoped plastic ablator at 1000 ps. Future work includes comparison of data with model at all times for both doped and undoped ablator samples. Omega laser target chamber