(Pre-School) C - Basics of stellar physics

• Sandro Bressan

Room: Fermi hall Basics of stellar physics. Overview on stellar structure and evolution. Main sequence, massive stars, supernovae, neutron stars

(Pre-School) B - Basics on cosmology

• Paolo Natoli

Room: Fermi hall Basics on Cosmology. Standard LCDM model for the particle students. Expansion and acceleration, dark matter and dark energy, the CMB

(Pre-School) A - Basics on particle physics

• Antonio Masiero

Room: Fermi hall Basics on particle physics. Structure of the Standard Model of particle physics

(Pre-School) B - Basics on cosmology

• Paolo Natoli

Room: Fermi hall Basics on Cosmology. Standard LCDM model for the particle students. Expansion and acceleration, dark matter and dark energy, the CMB

(Pre-School) C - Basics of stellar physics

• Sandro Bressan

Room: Fermi hall Overview on stellar structure and evolution. Main sequence, massive stars, supernovae, neutron stars

(Pre-School) A - Basics on particle physics

• Antonio Masiero

Room: Fermi hall Basics on particle physics. Structure of the Standard Model of particle physics

(Pre-School) A - Basics on particle physics

• Antonio Masiero

Room: Fermi hall Basics on particle physics. Structure of the Standard Model of particle physics

(Pre-School) C - Basics of stellar physics

• Sandro Bressan

Room: Fermi hall Overview on stellar structure and evolution. Main sequence, massive stars, supernovae, neutron stars

(Pre-School) A - Basics on particle physics

• Antonio Masiero

Room: Fermi hall Basics on particle physics. Structure of the Standard Model of particle physics

(Pre-School) B - Basics on cosmology

• Paolo Natoli

Room: Fermi hall Standard LCDM model for the particle students. Expansion and acceleration, dark matter and dark energy, the CMB

P1) Neutrino and its properties

• Marco Pallavicini

Room: Fermi hall Neutrino and its properties: flavours, cross section, mass, quantum numbers, Dirac and Majorana neutrinos, upper limit for magnetic moment, search for sterile neutrinos

P3) Neutrino oscillations

• Eligio Lisi

Room: Fermi hall Neutrino oscillation (solar and reactor neutrinos, neutrino beams, short and long baseline experiments-) CP violation in the lepton sector and mass ordering determination

P1) Neutrino and its properties

• Marco Pallavicini

Room: Fermi hall Neutrino and its properties: flavours, cross section, mass, quantum numbers, Dirac and Majorana neutrinos, upper limit for magnetic moment, search for sterile neutrinos

P3) Neutrino oscillations

• Eligio Lisi

Room: Fermi hall Neutrino oscillation (solar and reactor neutrinos, neutrino beams, short and long baseline experiments-) CP violation in the lepton sector and mass ordering determination

P1) Neutrino and its properties

• Marco Pallavicini

Room: Fermi hall Neutrino and its properties: flavours, cross section, mass, quantum numbers, Dirac and Majorana neutrinos, upper limit for magnetic moment, search for sterile neutrinos

P3) Neutrino oscillations

• Eligio Lisi

Room: Fermi hall Neutrino oscillation (solar and reactor neutrinos, neutrino beams, short and long baseline experiments-) CP violation in the lepton sector and mass ordering determination

A1) Solar, stellar and Supernova neutrinos.

• Aldo Ianni

Room: Fermi hall Solar, stellar and Supernova neutrinos. The key role of neutrino for Sun and stars physics.

P3) Neutrino oscillations

• Eligio Lisi

Room: Fermi hall Neutrino oscillation (solar and reactor neutrinos, neutrino beams, short and long baseline experiments-) CP violation in the lepton sector and mass ordering determination

P5) Neutrino nucleus interactions and cross section

• Kate Scholberg

Room: Fermi hall Neutrino nucleus interactions and cross section

A1) Solar, stellar and Supernova neutrinos.

• Aldo Ianni

Room: Fermi hall Solar, stellar and Supernova neutrinos. The key role of neutrino for Sun and stars physics.

A1) Solar, stellar and Supernova neutrinos.

• Aldo Ianni

Room: Fermi hall Solar, stellar and Supernova neutrinos. The key role of neutrino for Sun and stars physics.

A3) High energy cosmic neutrinos

• Elisa Resconi

Room: Fermi hall High energy cosmic neutrinos. IceCube and future measurements.

A3) High energy cosmic neutrinos

• Elisa Resconi

Room: Fermi hall High energy cosmic neutrinos. IceCube and future measurements.

P4) Neutrino mass determination

• Aleksei Lokhov

Room: Fermi hall Neutrino mass determination

C1) The role of the neutrinos in the LCDM

• Matteo Viel

Room: Fermi hall The role of the neutrinos in the LCDM. Overview and state of the art, tensions, open questions

Discussion Room: Fermi hall Exercises proposed by Kate Scholberg and Aldo Ianni

C1) The role of the neutrinos in the LCDM

• Matteo Viel

Room: Fermi hall The role of the neutrinos in the LCDM. Overview and state of the art, tensions, open questions

P2) Neutrinoless double beta decay

• Ezio Previtali

Room: Fermi hall Neutrinoless double beta decay

P2) Neutrinoless double beta decay

• Ezio Previtali

Room: Fermi hall Neutrinoless double beta decay

P4) Neutrino mass determination

• Aleksei Lokhov

Room: Fermi hall Neutrino mass determination

C1) The role of the neutrinos in the LCDM

• Matteo Viel

Room: Fermi hall The role of the neutrinos in the LCDM. Overview and state of the art, tensions, open questions

C2) Large Scale Structures and Neutrinos

• Enzo Branchini

Room: Fermi hall Large Scale Structures and Neutrinos. Neutrino mass estimate from LSS, Lyman-alpha forest

A2) Neutrinos from the violent universe

• Hans-Thomas Janka

Room: Fermi hall Neutrinos from the violent universe. Supernovae, Collapsing binaries, multi-messenger astrophysics; diffuse SN neutrino background

C2) Large Scale Structures and Neutrinos

• Enzo Branchini

Room: Fermi hall Large Scale Structures and Neutrinos. Neutrino mass estimate from LSS, Lyman-alpha forest

C2) Large Scale Structures and Neutrinos

• Enzo Branchini

Room: Fermi hall Large Scale Structures and Neutrinos. Neutrino mass estimate from LSS, Lyman-alpha forest

C3) Cosmic Microwave Background and neutrinos

• Douglas Scott

Room: Fermi hall Cosmic Microwave Background and neutrinos. Cosmological parameters from CMB, limits on neutrino mass and mass hierarchy, degeneracies.

A2) Neutrinos from the violent universe

• Hans-Thomas Janka

Room: Fermi hall Neutrinos from the violent universe. Supernovae, Collapsing binaries, multi-messenger astrophysics; diffuse SN neutrino background

A2) Neutrinos from the violent universe

• Hans-Thomas Janka

Room: Fermi hall Neutrinos from the violent universe. Supernovae, Collapsing binaries, multi-messenger astrophysics; diffuse SN neutrino background

C3) Cosmic Microwave Background and neutrinos

• Douglas Scott

Room: Fermi hall Cosmic Microwave Background and neutrinos. Cosmological parameters from CMB, limits on neutrino mass and mass hierarchy, degeneracies

C3) Cosmic Microwave Background and neutrinos

• Douglas Scott

Room: Fermi hall Cosmic Microwave Background and neutrinos. Cosmological parameters from CMB, limits on neutrino mass and mass hierarchy, degeneracies

C4) Neutrinos and the very early Universe

• Nicola Bartolo

Room: Fermi hall Neutrinos and the very early Universe: from inflation to the primordial Cosmic Neutrino Background

C4) Neutrinos and the very early Universe

• Nicola Bartolo

Room: Fermi hall Neutrinos and the very early Universe: from inflation to the primordial Cosmic Neutrino Background