Peggy McMahan Lawrence Berkeley Laboratory, Nuclear Science Division http://www.lbl.gov/abc/ 1 M.A.M.A. McMahan, February 2002 Outline I. A Bit of History II. Cyclotrons and other accelerators: The Legacy of E.O. Lawrence III. A Walk Around the Nuclear Wallchart: Nuclear Science in the 21st Century IV. Applications of Nuclear Science V. Resources a. Wallchart b. Web pages c. Cosmic Ray Detectors 2 M.A.M.A. McMahan, February 2002 3 M.A.M.A. McMahan, February 2002 I saw in a dream a table where all the elements fell into place as required. Awakening, I immediately wrote it down on a piece of paper. Only in one place did a correction later appear necessary. -Dmitri Mendeleev, 1869 4 M.A.M.A. McMahan, February 2002 The Beginning of Nuclear Science Poised on the threshold of a new century, scientists in the late 1800’s made discoveries which would change the course of science, history and medicine in the 20th Century. Henri Becquerel Marie and Pierre Curie 5 M.A.M.A. McMahan, February 2002 The Discovery of Radioactivity Henri Becquerel discovered radioactivity in 1896 when he was doing experiments on fluorescence of uranium-containing minerals. He was wrapping the minerals together with photographic plates in black paper and putting them in the sun. He thought the minerals absorbed energy from the sun and then emitted “x-rays” which gave an image of the minerals on the plate. But one cloudy week he put the samples in his desk drawer and a few days later developed the plate. Lo and behold, he saw a strong image anyway. The minerals were emitting x-rays without a source of external energy. Becquerel had discovered natural radioactivity. 6 M.A.M.A. McMahan, February 2002 Marie Curie Marie Curie ca 1920. Inset: Pierre Curie 7 Marie Curie, working on her thesis at the Sorbonne in Paris, together with her husband Pierre isolated the elements polonium and radium from ore containing uranium in 1898. In 1903, both Curies were awarded the physics Nobel prize for their discoveries. In 1911, Marie won an unprecedented second prize, in chemistry this time, for her chemical studies of the new elements. M.A.M.A. McMahan, February 2002 Types of Radioactivity In studies of natural radioactivity, Ernest Rutherford determined there were 3 kinds of radioactivity: In alpha decay, a nucleus emits an alpha particle (4He nucleus) with 2 neutrons and 2 protons In beta decay, a proton (or neutron) inside the nucleus transforms to a neutron (or proton), emitting a electron (or positron) and a neutrino (or antineutrino). In gamma decay, a nucleus keeps the same neutron and proton numbers, but de-excites by emitting gamma rays. 8 M.A.M.A. McMahan, February 2002 Proton # The Chart of the Nuclides: A “2-D” Periodic Table Neutron # 9 Nuclei have shells similar to the electron shells in an atom. The electron shells determine the atomic and chemical properties; the nuclear shells determine the nuclear properties. Nuclei with filled shells (a “magic” number of neutrons or protons) are more stable. M.A.M.A. McMahan, February 2002 Ernest Orlando Lawrence Lawrence at the controls of the 27” Cyclotron, about 1938. Lawrence’s first cyclotron, a few inches in diameter Ernest Orlando Lawrence invented the first cyclotron in 1929-31 in a small laboratory on the Berkeley campus. This was the foundation of the “Radiation Laboratory”. 10 M.A.M.A. McMahan, February 2002 Lawrence only thought he invented the cyclotron From a stone in a 200 BC Greek “hospital” in Asia Minor (modern Turkey) 11 M.A.M.A. McMahan, February 2002 What is an accelerator? If a charged particle goes through an electric field it gets accelerated. The amount of acceleration depends on the strength of the electric field. A simple vacuum tube accelerator Scientists/engineers tried to put more and more voltage across a gap to make an electron field to accelerate a particle to 1 million electron volts (MeV). When they couldn’t get any higher, they tried to put a bunch of gaps together, so that the particle would get successively accelerated. 12 M.A.M.A. McMahan, February 2002 Lawrence’s breakthrough ● ● 13 Lawrence took the idea of successive accelerations from Wideroe and suggested “rolling up” the linear accelerator into a circle. Lawrence’s 11” cyclotron reached the sought-after goal of 1 MeV acceleration. M.A.M.A. McMahan, February 2002 A Bit of Local History ● ● ● ● ● 14 E.O. Lawrence invented the Cyclotron in 1931 on campus He rapidly moved up in size to 27”, 36” and finally 60” cyclotrons. The 60” cyclotron was built to make medical isotopes. LBNL came into being when he conceived the 184” Cyclotron, too large to build on campus The 88-Inch Cyclotron, in operation since 1962, is a third generation, “sector-focused” cyclotron Many years later, the 88-Inch Cyclotron is the last nuclear physics accelerator left on the site M.A.M.A. McMahan, February 2002 15 M.A.M.A. McMahan, February 2002 How a cyclotron works 16 M.A.M.A. McMahan, February 2002 The 88-Inch Cyclotron Facility 17 M.A.M.A. McMahan, February 2002 Gammasphere - the world’s most powerful detector array to measure gamma rays A beam particle hits a target nucleus inside Gammasphere The two nuclei fuse to make a hot “compound nucleus” which can be elongated and rotating The compound nucleus cools down by emitting neutrons and protons The rotating nucleus emits gamma rays which are detected in Gammasphere 18 M.A.M.A. McMahan, February 2002 The Expansion of the Universe Relativistic Collisions (RHIC) 19 Medium Energy (JLAB) Low Energy (small accelerators; RIA) M.A.M.A. McMahan, February 2002 Nuclear Astrophysics (small accelerators; nonaccelerator) Phases of Nuclear Matter 20 M.A.M.A. McMahan, February 2002 The Structure of the Nucleus 21 M.A.M.A. McMahan, February 2002 Nuclei at the Extreme of Mass Natural Radioactivity 22 Man-made Radioactivity: the heaviest elements M.A.M.A. McMahan, February 2002 Nuclei at the neutron and proton “driplines” Proton # The formation of elements in supernovae explosions follows this path (maybe) Neutron # 23 The Rare Isotope Accelerator, RIA, the next proposed large accelerator at the DOE, will accelerate radioactive species in order to study nuclear astrophysics and the formation of the elements. M.A.M.A. McMahan, February 2002 Neutrinos from the Sun •Nuclear reactions in the sun produce photons and electron neutrinos •Early experiments measured too few neutrinos to be explained by reaction models. 24 •First results from SNO (2001) show that the electron neutrinos are oscillating into other flavors (µ,τ) before reaching the detector. This proves neutrinos have mass! M.A.M.A. McMahan, February 2002 Applications of Nuclear Science 25 M.A.M.A. McMahan, February 2002 Resources for Teachers ● 26 The Cosmic Connection http://www.lbl.gov/abc/cosmic/ M.A.M.A. McMahan, February 2002 Viewing the x-ray spectrum of 63 elements http://ie.lbl.gov/xray/ 27 M.A.M.A. McMahan, February 2002