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The ALPS Experiment PDF

102 Pages·2010·7.2 MB·English
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The ALPS Experiment DDaarrkk MMaatttteerr aanndd PPaarrttiiccllee Physics at Lowest Energies A. Lindner, DESY DESY Summer Student Lecture, 30 July 2010 Today’s Agenda > The ALPS Lecture which is the last one of the common lectures in the past two weeks. Therefore it might be a good opportunity to ask questions and rise some items. > Question Time!  Nagging issues related to the common lectures.  Curiosity concerning DESY in general.  Everything you wanted to know about DESY physics but were afraid to ask (answers not guaranteed).  Other items? > “Hands on” with Cosmic Rays and a tour to the ALPS? Axel Lindner | Summer Students 2010 | ALPS | Page 2 The ALPS Lecture > An Introduction to the Axion > Dark Stuff in the Universe > From Axions to ALPs and WISPs > How to search for WISPs > The ALPS Experiment at DESY > Outlook on possible future Activities > Summary Axel Lindner | Summer Students 2010 | ALPS | Page 3 Table of Contents > An Introduction to the Axion > Dark Stuff in the Universe > From Axions to ALPs and WISPs > How to search for WISPs > The ALPS Experiment at DESY > Outlook on possible future Activities > Summary Axel Lindner | Summer Students 2010 | ALPS | Page 4 The Standard Model of Constituents and Forces / Constituents: s e b u > Quarks c / k u . c > Leptons a . p p d i r g . w Forces: w w / > electromagnetic :/ p t t h > strong > weak > gravitation Only the Higgs boson is missing! LHC is on the way to probe its existence. Axel Lindner | Summer Students 2010 | ALPS | Page 5 The Standard Model of Constituents and Forces / Constituents: With these few s e b constituents and forces all u > Quarks c / k phenomena observed on u . c > Leptons a earth can be . p p d described (in principle). i r g . w Forces: w w Since more than 30 years / > electromagnetic :/ p t there is not a single t h > strong particle physics experiment > weak really questioning the > gravitation Standard Model. Only the Higgs boson is missing! LHC is on the way to probe its existence. Axel Lindner | Summer Students 2010 | ALPS | Page 6 A Flaw in the Standard Model? The neutron has a strange property: It consists of three charged quarks, but does not show any static electric dipole moment. http://www.lbl.gov/Science-Articles/Archive/sabl/2006/Oct/3.html http://en.wikipedia.org Why do the wave functions of the three quarks exactly cancel out any observable static charge distribution in the neutron? Axel Lindner | Summer Students 2010 | ALPS | Page 7 A Flaw in the Standard Model? Naively one expects for the neutron electric dipole moment: ml ht 3. ct/ O 6/ 0 0 2 bl/ a s d  10-15 e·cm. m e/ v n-QCD c hi c 5 Ar -1 s/ 0 e 1 cl rti  A - e c n e ci S v/ o g bl. w.l w w p:// htt The data show: d < 10-26 e·cm! n-data How to explain the difference of at least 11 orders of magnitude? Axel Lindner | Summer Students 2010 | ALPS | Page 8 Eleven Orders of Magnitude … expecting a planet and finding the nanoscale … Axel Lindner | Summer Students 2010 | ALPS | Page 9 Two Possibilities > The vanishing electric dipole moment of the neutron is just accidental. The parameters of QCD are “fine-tuned”, nothing remains to be explained. A physicist’s nightmare: > Can one think of any explanation? If yes, how to confirm this? Axel Lindner | Summer Students 2010 | ALPS | Page 10

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Dark Matter and. Particle. Particle Physics at Lowest Energies. A. Lindner, DESY. The ALPS Experiment. DESY Summer Student Lecture, 30 July 2010 .. pulse from SN and cosmic microwave background radiation for example. > Direct: ▫ Search for axions from the sun. (CAST at CERN). ▫ Search for.
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