10616298 | QUANTUM MECHANICS AND STATISTICAL MECHANICS | 1st | 12 | ITA |
Educational objectives GENERAL OBJECTIVES:
The course aims at introducing the basic notions of nonrelativistic quantum mechanics and of statistical mechanics and illustrating their application to symple physical systems. At the end of the course, students will possess the fundamentals of both theories. They will have also acquired the skills necessary to solve Schrodinger’s equation and evaluate the partition function of simple systems of noninteracting particles obtaining the corresponding physical properties.
SPECIFIC OBJECTIVES:
A - Knowledge and understanding
OF 1) To know the basic notions of nonrelativistic quantum mechanics for a single particle or a system of noninteracting particles.
OF 2) To understand the notion of spin and the composition of angular momenta.
OF 3) To know the perturbation theory, time dependent and time independent, also in the presence of degeneracy.
OF 4) To understand the connection between particle spin and particle exchange symmetry for a quantum state.
OF 5) To know the basic notions of statistical mechanics for systems of noninteracting particles, classical or quantum.
OF 6) To understand the notions of micro- and macrostate as well as that of equilibrium state in the case of microcanonical, canonical and grancanonical ensembles.
OF 7) To know the main state functions and their relations
B - Application skills
OF 8) To be able to face with conceptual problems among the arguments discussed.
OF 9) To be able to solve simple problems with analytical techniques.
OF 10) To be able to lay out a problem to be solved with numerical techniques.
C - Autonomy of judgment
OF 11) To be able to establish a bidirectional link between mathematical solutions of a problem and the physical properties of the corresponding system.
D - Communication skills
OF 12) To be able to communicate in a synthetic but comprehensive way the solution of problems and its logical structure.
E - Ability to learn
OF 13) Have the ability to consult different textbooks using different notations.
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1038469 | ASTROPHYSICS | 1st | 6 | ITA |
Educational objectives GENERAL OBJECTIVES:
The course is a general introduction to astrophysics. It aims at the description the most important physical mechanisms and phenomena at work in the universe: stellar, interstellar, galactic, extragalactic and cosmological. The focus is on the modelling of astrophysical and cosmological phenomena, and on the use of physical laws in the interpretation of astrophysical and cosmological observations.
SPECIFIC OBJECTIVES:
A - Knowledge and understanding
OF 1) To know the stellar phenomenology and understand it in terms of the different physical mechanisms of energy production. Understand the stellar evolution, as described by the fundamental equations of stellar structure.
OF 2) To know the phenomenology of the insterstellar medium (plasmas, gases, dust) and understand it in terms of physical mechanisma of emission and absorption.
OF 3) To know the phenomenology of the Galaxy and of the galaxies in the universe, and understand it in terms of the physical phenomena at work.
OF 4) To know the cosmological phenomenology, the observables and their use in the development of a physical model of the universe at large scales. To understand the cosmological evolution of the universe in the homogenous isotropic approximation using physics and in particular gravitation.
B - Application skills
OF 5) To be able to explain astrophysical and cosmological measurements, and use them to constrain the physical model of the system under study, understanding its nature.
C - Autonomy of judgment
OF 6) To master the acquired know-how, and use it in the solution of basic problems in astrophysics and cosmology, and in the understanding of the specialized literature.
D - Communication skills
E - Ability to learn
OF 7) To be able to understand specialistic papers in order to deepen the knowledge of particular topics introduced during the course.
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10599983 | Astrophysical laboratory | 1st | 9 | ITA |
Educational objectives GENERAL OBJECTIVES:
The objectives of this course are to provide the knowledge of the astronomical observation techniques, and of theastronomical instrumentation as well as the choice of the astronomical observables. Furthermore, the course aimsat using, and understanting the characteristics of, astrophysical instrumentation for laboratory classes andradio/optical observations. The student will understand the importance of the calibration and of the noisemitigation techniques through a series of experimental classes both in the laboratory and at the radioastronomy/optical-astronomy facilities on the roofs of the Physics department at Sapienza. Basic concepts ofastronomical optics, electronics, signal theory, cryogenics, interferometry, spectroscopics, polarimetry, will bepresented as well as the state of the art of radio, mm, sub-mm, IR, optical, UV, X, gamma instrumentation.
SPECIFIC OBJECTIVES:
A -Knowledge and understanding
OF 1) Know the fundamentals of astronomical observations
OF 2) To know the fundamentals of the functioning of astrophysical radiation detectors
OF 3) Understand the use of astrophysical radiation detection techniques
B -Application skills
OF 4) Knowing how to deduce the characteristics of an astrophysical observation
OF 5) Solve problems related to noise
OF 6) Be able to apply noise reduction techniques / methods
C -Autonomy of judgment
OF 7) Being able to evaluate the best way to perform a measurement
OF 8) Integrate the acquired knowledge in order to establish the best observational techniqueD -Communication skills
OF 9) Knowing how to communicate the results of one's work in writing in laboratory reports
OF 10) Knowing how to communicate about known and unknown problemsE -Ability to learn
OF 11) Have the ability toconsult electronic components datasheets
OF 12) Have the ability to evaluate the adequacy of an astrophysics instrument
OF 13) Be able to conceive and develop an astronomical project
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Astrophysical laboratory II | 1st | 6 | ITA |
Educational objectives GENERAL OBJECTIVES:
The objectives of this course are to provide the knowledge of the astronomical observation techniques, and of theastronomical instrumentation as well as the choice of the astronomical observables. Furthermore, the course aimsat using, and understanting the characteristics of, astrophysical instrumentation for laboratory classes andradio/optical observations. The student will understand the importance of the calibration and of the noisemitigation techniques through a series of experimental classes both in the laboratory and at the radioastronomy/optical-astronomy facilities on the roofs of the Physics department at Sapienza. Basic concepts ofastronomical optics, electronics, signal theory, cryogenics, interferometry, spectroscopics, polarimetry, will bepresented as well as the state of the art of radio, mm, sub-mm, IR, optical, UV, X, gamma instrumentation.
SPECIFIC OBJECTIVES:
A -Knowledge and understanding
OF 1) Know the fundamentals of astronomical observations
OF 2) To know the fundamentals of the functioning of astrophysical radiation detectors
OF 3) Understand the use of astrophysical radiation detection techniques
B -Application skills
OF 4) Knowing how to deduce the characteristics of an astrophysical observation
OF 5) Solve problems related to noise
OF 6) Be able to apply noise reduction techniques / methods
C -Autonomy of judgment
OF 7) Being able to evaluate the best way to perform a measurement
OF 8) Integrate the acquired knowledge in order to establish the best observational techniqueD -Communication skills
OF 9) Knowing how to communicate the results of one's work in writing in laboratory reports
OF 10) Knowing how to communicate about known and unknown problemsE -Ability to learn
OF 11) Have the ability toconsult electronic components datasheets
OF 12) Have the ability to evaluate the adequacy of an astrophysics instrument
OF 13) Be able to conceive and develop an astronomical project
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1039018 | FLUIDODYNAMICS FOR ASTROPHYSICS | 1st | 6 | ITA |
Educational objectives GENERAL OBJECTIVES:
The main aim of the course is to introduce students to the basic equations describing fluid flows by mean of a careful mathematical treatment of the involved physical aspects. The Lagrangian and Eulerian views will be introduced and their applications to both ideal and realistic fluids and gases presented and discussed. In particular, the unavoidable numerical treatment of dynamics of gases and fluids in astrophysical conditions will be discussed. The, Lagrangian, Smooth Particle Hydrodynamics method (SPH) will be presented as one of the best suited to applications where a body force, like gravity, is present.
At the end of the course the students should be able to deal with methods and basic techniques to deal with problems of dynamics of fluids in both terrestrial and astrophysical context.
SPECIFIC OBJECTIVES:
A - Knowledge and understanding
OF 1) To know the constitutive equations underlying fluid dynamics and energetics.
OF 2) To understand the physical processes that control the evolution of fluids, from gases to liquids and plasmas.
OF 3) To understand the differences of the fluid dynamics in a terrestrial context respect to the astrophysical one.
B - Application skills
OF 4) To be able to apply, both on a theoretical and numerical side, the acquired knowledge to the interpretation and explanation of phenomena involving fluids in terrestrial and astrophysical context.
C - Autonomy of judgment
OF 5) To be able to evaluate the coherence between the physical framework and the mathematical scheme of representation adopted.
D - Communication skills
To be able to describe in a clear and critical way the contents of the various topics approached in the course.
E - Ability to learn
OF 6) Have the ability to deal with available didactic and scientific reference textbooks and papers in order to further explore some of the topics introduced during the course.
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1018976 | OPTICS AND LABORATORY | 2nd | 9 | ITA |
Educational objectives GENERAL OBJECTIVES:
The student will acquire knowledge of the fundamental principles and laws of Classical Optics, with regards to general phenomena, such as interference, diffraction and polarization of light. These phenomena will be also investigated in laboratory sessions by using advanced didactic set-ups. The student will learn how to use the basic principles of Optics to solve simple problems related to the knowledge acquired during the course. At the end of the course, the students will develop quantitative reasoning abilities and problem-solving skills, which represent the basis to study, model and understand light propagation and interaction with matter at a fundamental level.
Furthermore, thanks to the laboratory sessions, the student will develop practical ability to use optical set-ups as well as to convey the observations made during the experiments via laboratory reports. A direct interaction with the teacher will be also a plus during the execution of the experiments.
SPECIFIC OBJECTIVES:
A - Knowledge and understanding
OF 1) Understand the fundamentals of physical optics (electromagnetic waves)
OF 2) Understand the fundamentals of optics in linear media (isotropic and anisotropic dielectrics)
OF 3) To understand the language of optics
B - Application skills
OF 4) To be able to assemble simple optical experiments
OF 5) To be able to align an optical interferometer
OF 6) To be able to measure optical intensity (photodiodes)
OF 7) To be able to measure and control light polarization states
C - Autonomy of judgment
OF 8) To be able to evaluate the best way of performing an experimental measurement
D - Communication skills
OF 9) To know how to communicate in written reports the results the experimental work
OF 10) To know how to discuss the characteristics and functionalities of simple optical schemes
E - Ability to learn
OF 11) Being able to consult optical components datasheets
OF 12) Being able to design a of simple optical schemeanalog and digital circuits
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1012093 | STRUCTURE OF MATTER | 2nd | 6 | ITA |
Educational objectives GENERAL OBJECTIVES:
The goal of the course is to study the foundations of material’s structure, providing the basis of atomic and molecular physics, with an elementary introduction to solid state physics, starting from knowledge and methods of quantum mechanics. The student, at the end of the course, will acquire basic concepts to determine energy eigenvalues ang eigenstates of atomic and molecular systems unser external fields. The developed know-how will be fundamental for the advanced condensed matter and solid state physics courses.
SPECIFIC OBJECTIVES:
A - Knowledge and understanding
OF 1) To know foundations of atomic and molecular physics, and basics elements of solid state physics
OF 2) To understand energy spectra and eigenstates of atomic, molecular and solid state systems.
OF 3) Undesratnd principles of light-matter interaction.
B - Application skills
OF 4) Learn how to apply principles of quantum mechanics do describe atoms and molecules.
OF 5) Solve problems related to atomic and molecular spectra
OF 6) To be able to apply perturbative and variational techniques to evaluate eigenvalues and eigenstates at atoms and molecules
C - Autonomy of judgment
OF 7) To be able to apply in the future the acquired skills to the more general context of condensed matter physics
D - Communication skills
OF 8) To know how to communicate the critical steps necessary to solve elementary problems dealing with material structure
E - Ability to learn
OF 10) Have the ability to autonomously consult basic textbooks and in some cases scientific articles to expand the knowledge developed in the course
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10599983 | Astrophysical laboratory | 2nd | 9 | ITA |
Educational objectives GENERAL OBJECTIVES:
The objectives of this course are to provide the knowledge of the astronomical observation techniques, and of theastronomical instrumentation as well as the choice of the astronomical observables. Furthermore, the course aimsat using, and understanting the characteristics of, astrophysical instrumentation for laboratory classes andradio/optical observations. The student will understand the importance of the calibration and of the noisemitigation techniques through a series of experimental classes both in the laboratory and at the radioastronomy/optical-astronomy facilities on the roofs of the Physics department at Sapienza. Basic concepts ofastronomical optics, electronics, signal theory, cryogenics, interferometry, spectroscopics, polarimetry, will bepresented as well as the state of the art of radio, mm, sub-mm, IR, optical, UV, X, gamma instrumentation.
SPECIFIC OBJECTIVES:
A -Knowledge and understanding
OF 1) Know the fundamentals of astronomical observations
OF 2) To know the fundamentals of the functioning of astrophysical radiation detectors
OF 3) Understand the use of astrophysical radiation detection techniques
B -Application skills
OF 4) Knowing how to deduce the characteristics of an astrophysical observation
OF 5) Solve problems related to noise
OF 6) Be able to apply noise reduction techniques / methods
C -Autonomy of judgment
OF 7) Being able to evaluate the best way to perform a measurement
OF 8) Integrate the acquired knowledge in order to establish the best observational techniqueD -Communication skills
OF 9) Knowing how to communicate the results of one's work in writing in laboratory reports
OF 10) Knowing how to communicate about known and unknown problemsE -Ability to learn
OF 11) Have the ability toconsult electronic components datasheets
OF 12) Have the ability to evaluate the adequacy of an astrophysics instrument
OF 13) Be able to conceive and develop an astronomical project
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Astrophysical laboratory I | 2nd | 3 | ITA |
Educational objectives GENERAL OBJECTIVES:
The objectives of this course are to provide the knowledge of the astronomical observation techniques, and of theastronomical instrumentation as well as the choice of the astronomical observables. Furthermore, the course aimsat using, and understanting the characteristics of, astrophysical instrumentation for laboratory classes andradio/optical observations. The student will understand the importance of the calibration and of the noisemitigation techniques through a series of experimental classes both in the laboratory and at the radioastronomy/optical-astronomy facilities on the roofs of the Physics department at Sapienza. Basic concepts ofastronomical optics, electronics, signal theory, cryogenics, interferometry, spectroscopics, polarimetry, will bepresented as well as the state of the art of radio, mm, sub-mm, IR, optical, UV, X, gamma instrumentation.
SPECIFIC OBJECTIVES:
A -Knowledge and understanding
OF 1) Know the fundamentals of astronomical observations
OF 2) To know the fundamentals of the functioning of astrophysical radiation detectors
OF 3) Understand the use of astrophysical radiation detection techniques
B -Application skills
OF 4) Knowing how to deduce the characteristics of an astrophysical observation
OF 5) Solve problems related to noise
OF 6) Be able to apply noise reduction techniques / methods
C -Autonomy of judgment
OF 7) Being able to evaluate the best way to perform a measurement
OF 8) Integrate the acquired knowledge in order to establish the best observational techniqueD -Communication skills
OF 9) Knowing how to communicate the results of one's work in writing in laboratory reports
OF 10) Knowing how to communicate about known and unknown problemsE -Ability to learn
OF 11) Have the ability toconsult electronic components datasheets
OF 12) Have the ability to evaluate the adequacy of an astrophysics instrument
OF 13) Be able to conceive and develop an astronomical project
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Elective course | 2nd | 6 | ITA |
Educational objectives The aim of the course is to enable students to enrich the knowledge of curricular courses with topics of their choice.
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AAF1001 | FINAL EXAM | 2nd | 3 | ITA |
Educational objectives The final exam consists of the presentation of a report on the activities conducted during the stage/thesis. The preparation for this exam implies skills related to the presentation of her/his work, and the capability to discuss and argue with an audience fully aware of the topics presented.
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