References 485
[12A10] Agafonova, N.: et al., (OPERA Coll.): Observation of a first
candidate in the
OPERA experiment in the CNGS beam. Phys. Lett. B 691, 138–145 (2010). Also:
arXiv:1006.1623 [hep-ex]
Chapter 13
[13P74] Pati, C., Salam, A.: Lepton number as the fourth color. Phys. Rev. D 10, 275 (1974)
[13G84] Giacomelli, G.: Magnetic monopoles. La Rivista del Nuovo Cimento 7(12), 1 (1984)
[13D94] De Boer, W.: Grand Unified theories and supersymmetry in particle physics and cos-
mology. Prog. Part. Nucl. Phys. 33, 201 (1994). Also: arXiv:hep-ph/9402266v5
[13L94] Lopez, J., Nanopoulos, D.V., Zichichi, A.: A layman’s guide to SUSY GUT. La Rivista
del Nuovo Cimento 17(2), 1 (1994). Also in: http://cdsweb.cern.ch/record/255084/
[13B00] De Bernardis, P., et al.: A flat universe from high-resolution maps of the cosmic
microwave background radiation. Nature 404, 955 (2000)
[13G00] Greene, B.: The Elegant Universe: Superstrings, Hidden Dimensions, and the Quest for
the Ultimate Theory. Vintage Series, Random House Inc., New York (2000) ISBN: 978-
0375708114
[13S04] Riess, A.G., et al., (Supernova Search Team Coll.): Type Ia supernova discoveries at z>1
from the Hubble space telescope: Evidence for past deceleration and constraints on dark
energy evolution. Astrophys. J. 607, 665–687 (2004). Also: astro-ph/0402512.
[13W07] Spergel, D.N., et al., (WMAP Coll.): Wilkinson microwave anisotropy probe (WMAP)
three year results: Implications for cosmology. Astrophys. J. Suppl. 170, 377 (2007).
Also: astro-ph/0603449.
[13B08] Bernabei, R., et al., (DAMA Coll.): First results from DAMA/LIBRA and combined
results with DAMA/NaI. Eur. Phys. J. C 56, 333 (2008). Also: arXiv:0804.2741
[astro-ph]
[13C10] Chiarusi, T., Spurio, M.: High-energy astrophysics with neutrino telescopes. Eur. Phys.
J. C 65, 649–710 (2010)
[13M10] J. Adam et al. (MEG Collaboration). A limit for the ! e decay from the MEG
experiment. Nucl. Phys. B834 (2010), 1–12
[13w1] The SUSY LEP working group. http://lepsusy.web.cern.ch/lepsusy/www/
[13w2] The Higgs LEP working group. http://lephiggs.web.cern.ch/LEPHIGGS/papers/index.
html
Chapter 14
[14B57] Burbidge, E.M., Burbidge, G.R., Fowler, W.A., Hoyle, F.: Synthesis of the elements
in stars. Rev. Mod. Phys. 29, 547 (1957). This historical article is jokingly referred as
B
2
FH
[14S83] Simpson, J.A.: Elemental and isotopic composition of the galactic cosmic rays. Annu.
Rev. Nucl. Part. Sci. 33, 323 (1983)
[14T98] Truran, J.W.: The age of the universe from nuclear chronometers. Proc. Natl. Acad. Sci.
U.S.A. 95, 18–21 (1998). This paper was presented at a colloquium entitled The Age of
the Universe, Dark Matter, and Structure Formation whose proceedings are available at
http://www.nap.edu/catalog.php?record
id=6237
[14w1] http://www.physics.brocku.ca/applets/MassSpectrometer/index.html
[14w2] National Nuclear Data Center, information extracted from the NuDat 2 database. http://
www.nndc.bnl.gov/nudat2/
[14w3] Bertsch, G., Bulgac, A., Luo, A., McDaniel, C.: Liquid Drop Model of Nuclear Binding
Energy. http://128.95.95.61/
intuser/ld3.html
[14w4] Fusion for Energy (F4E) is the European Union’s Joint Undertaking for ITER and the
Development of Fusion Energy. http://fusionforenergy.europa.eu/