## Proceedings of the International School of Physics "Enrico Fermi.", Volume 11N. Zanichelli, 1960 - Nuclear physics |

### From inside the book

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Page 23

28 ) ) , always

an independent operator there is also the intrinsically different possibility ( II . 39 )

P2 = 1 ; in the presence of Majorana fields eq . ( II . 39 ) cannot occur . Whether ...

28 ) ) , always

**possible**to obtain eq . ( II . 37 ) ( or n = + 1 ) . In theories where F isan independent operator there is also the intrinsically different possibility ( II . 39 )

P2 = 1 ; in the presence of Majorana fields eq . ( II . 39 ) cannot occur . Whether ...

Page 55

In other words : is it at all

say , in conjunction with the emission of an electron from those emitted in

conjunction with the emission of an positron ? An experimental test of this

problem was ...

In other words : is it at all

**possible**to distinguish between the neutrinos emitted ,say , in conjunction with the emission of an electron from those emitted in

conjunction with the emission of an positron ? An experimental test of this

problem was ...

Page 189

Let evolution continue , as well catalyzed as

removal of heat as efficient as

eject matter . It can ' t radiate photons . It can ' t emit neutrinos . It comes into the

absolutely ...

Let evolution continue , as well catalyzed as

**possible**, with means for theremoval of heat as efficient as

**possible**. Ultimately the star gets tired . It can ' teject matter . It can ' t radiate photons . It can ' t emit neutrinos . It comes into the

absolutely ...

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### Contents

GENERALITÀ | 1 |

PARTE PRIMA Problemi teorici | 9 |

PARTE SECONDA Correlazioni angolari polarizzazioni e decadimenti beta | 197 |

4 other sections not shown

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### Common terms and phrases

allowed angle angular assumed calculated charge classical combination completely component connection conservation consider constant contribute correlation corresponding coupling curvature decay defined density dependence derived described determination direction discussed effects electric electromagnetic field electron element elementary emission energy equations example existence experiment experimental expression factor Fermi field final finds formula function geometrodynamics geometry give given gravitational histories initial interaction invariance known leads limit magnetic mass matrix means measured metric modes momentum neutrino neutron nuclei nucleons observed obtained operators pairs parity particle phase Phys physics polarization possible present principle problem properties purely quantity quantum quantum mechanics question radiation ratio reason reference relation relativity requires respect result scattering shown shows solution space spin symmetry Table theory transformation transitions universe vector wave weak zero