Tales from Nuclear Science Nov 2012 1 E Beise UMD The Medusa Nebula NASAs Astronomy picture of the day Oct 25 2012 copyright K Crawford Rancho del Sol Observatory Betsy Beise Identifying the big questions ID: 497100
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Slide1
The Matter of Our Matter:
Tales from Nuclear Science
Nov 2012
1
E. Beise UMD
The Medusa Nebula (NASA’s Astronomy picture of the day Oct 25, 2012)
copyright K. Crawford (Rancho del Sol Observatory)
Betsy BeiseSlide2
Identifying the big questions
and the tools to answer them
Nov 2012
2
E. Beise UMD
Nuclear Science Advisory Committee (NSAC)
Long Range Plan 2007National Academies2012
http://science.energy.gov/np/nsac/
http://www.nap.edu/catalog.php?record_id=13438Slide3
100 years of nuclear science
Nov 2012
3
E. Beise UMD
Ernest Rutherford
1871-1937
Nobel Prize in Chemistry, 1908
atomic nucleus
identified in 1911
"for his investigations into the disintegration of the elements, and the chemistry of radioactive substances"
.Slide4
Harriet Brooks
1876-1933
naturally occurring Uranium
Radon gas
more protons
more neutrons
beta
decay
(neutron turns into a proton, releases an
electron
… and antineutrino)
Thorium
Nov 2012
E. Beise UMD
4Slide5
The tale of visible matter
Nov 20125E. Beise UMD
first few
microseconds
first few
minutes
billions of
years later ….
once upon
a time….
How were the elements such as gold, platinum, uranium (or anything heavier than iron) created ?
Why are certain elements stable and others unstable?Slide6
http://education.jlab.org/itselemental
The Periodic Table of Elements
8
O
Oxygen
16
Nov 2012
E. Beise UMD
6
Maria
Goeppert-Mayer
1963Slide7
Marguerite
Perey1909 – 1975
87Fr
Francium223
Lise
Meitner
1878 - 1968
91
Pa
Protactinium
231
1939
explanation of nuclear fission
Tales of heavy nuclei
Nov 2012
7
E. Beise UMD
1939
discovered Francium
1921
discovered Protactinium
109
Mt
Meitnerium
278
first produced in 1982Slide8
Nov 2012
E. Beise UMD
8Slide9
simulation based on measured nuclear m
asses and
b
eta-decay rates
(courtesy A.
Aprahamian
, Notre Dame)Creation of heavy elements:
rapid capture of neutrons
Nov 2012
9
E. Beise UMD
many elements made from beta decay
Heaviest
elements thought to be
made from rapid neutron capture (r-process)
Where are they made? How?
Ni
SnSlide10
The National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University
Nov 2012
10
E. Beise UMD
K500
A1900
production
target
ion sources
coupling
line
p/p = 5%
transmission
of 65% of the
produced
78
Ni
86
Kr
14+
,
12 MeV/u
86
Kr
34+
,
140 MeV/u
Example:
86
Kr
→
78
Ni
productionSlide11
Facility for Rare Isotope Beams (FRIB)
Nov 201211E. Beise UMD
Preparing for construction at MSU
number of protonsSlide12
Tales of creation
Nov 201212E. Beise UMD
first few
microseconds
first few
minutes
billions of
years later ….
once upon
a time….
What were the properties of matter in the earliest stages of the universe, just after the quarks and gluons were created?
How did the quarks and gluons combine to form protons and neutrons?Slide13
The Relativistic Heavy Ion Collider
Brookhaven National Laboratory, (Long Island, NY)Nov 201213
E. Beise UMD
STAR detectorSlide14
Colliding Gold nuclei at RHIC
Nov 201214E. Beise UMD
STAR detector eventSlide15
Quark-gluon plasma seems to be nature’s most perfect liquid
Nov 2012
E. Beise UMD
15Slide16
the tale of formation
Nov 201216E. Beise UMD
first few
microseconds
first few
minutes
billions of
years later ….
once upon
a time….
How do we describe the properties of neutrons and protons based on the fundamental force that holds them together? Slide17
Proton = up + up + down
charge = 2/3 + 2/3 – 1/3 = 1
neutron = up + down + down
charge = 2/3 – 1/3 – 1/3 = 0
quarks and gluons in
protons and neutrons
Nov 2012
17
E. Beise UMD
almost all the mass comes from the gluons – the energy field – not the 3 quarks
nucleus
Theory and Computation
1
H
Hydrogen
1.00794Slide18
Looking inside through scattering
(a la Rutherford)Nov 201218
E. Beise UMD
Particles sometimes act like waves
The higher the momentum, the smaller the wavelength, the shorter distances can be seen.
microscopeSlide19
Jefferson Laboratory
(Newport News, VA)
East Arc Tunnel Magnets
Energy doubling upgrade in progress underway
Nov 2012
E. Beise UMD
19Slide20
target
detector
beam
Nov 2012
E. Beise UMD
20Slide21
Cryogenic Targets
Nov 201221E. Beise UMD
Hall C targets
liquid Hydrogen
liquid deuterium
solid targets
G0 targetSlide22
G
0 beam girder
Superconducting Magnet
(SMS)
FPDs
Spokesman
Target module
CED+Cherenkov
G0 Detector in Hall C
at Jefferson Lab
Nov 2012
E. Beise UMD
22Slide23
MIT-Bates linear accelerator, Middleton, MA
North Hall
my PhD Thesis
experiment
county jail
23
E. Beise, U MarylandSlide24
Proton’s charge and magnetism distributions are very different
Proton charge and magnetismNov 2012
24
E. Beise UMD
proton
Carlson &
Vanderhaeghen
, Phys. Rev.
Lett
. 100 (2008) 032004
Since
JLab
Before
JLab
smaller distances
neutronSlide25
Societal Applications
Nov 2012
25
E. Beise UMD
Border Protection
High Performance Computing
Energy
medical imaging
isotope production
Nuclear Forensics
Safety and securing of nuclear weapons
accelerator technologySlide26
Positron Emission Tomography
Nov 2012
26
E. Beise UMD
Radioactive
18
F embedded in a molecule with glucose, can be readily absorbed by the brain(fludeoxyglucose – 18F-FDG)
Brain image from D. Wilson, British Columbia Cancer AgencySlide27
Magnetic Resonance Imaging
with polarized gasNov 201227
E. Beise UMD
p
p
n
nuclear spin of
3
He gas aligned in magnetic field
MRI magnetic field sees the gas in patient’s
lungs: real time lung function
lung image from Univ. of VirginiaSlide28
Detecting very low levels of radioactivity
Nov 201228E. Beise UMD
J. Diaz et al., Jour.
Env
. Radioactivity, 102, 2011
In Seattle, Washington
Fukushima Earthquake, March 2011Slide29
Nov 2012
29E. Beise UMD
LUX:
Dark Matter search
EXO: 0
nbb
search
UMD-NIST collaborationSlide30
Nov 2012
E. Beise UMD
30Slide31
Nov 2012
E. Beise UMD31