{"id":null,"code":"TÄHT7036","name":{"valueFi":"High-energy Astrophysics","valueEn":"High-energy Astrophysics","valueSv":"High-energy Astrophysics"},"credits":8.0,"minCredits":8,"maxCredits":8,"tags":[],"createdAt":1790534678399,"contentList":[{"title":{"valueFi":"Osaamistavoitteet","valueEn":"Learning outcomes","valueSv":""},"content":{"valueFi":"","valueEn":"At the end of the course, students should be able to: \r\n- describe the physics of compact stars and derive the mass-radius relationship for compact stars assuming degenerate electron or neutron pressure; \r\n- outline the main methods of measuring masses, radii and spins of compact stars; \r\n- show the Galactic distribution of different classes of compact stars; \r\n- discuss the period-period derivative relation for pulsars and place there different classes of pulsars; \r\n- describe different methods of the magnetic field determination of compact stars; \r\n- develop self-study skills; \r\n- solve problems on topics in the syllabus; \r\n- read, understand and be able to answer questions on scientific refereed articles in the field of high-energy astrophysics.","valueSv":""}},{"title":{"valueFi":"Sisältö","valueEn":"Content","valueSv":""},"content":{"valueFi":"","valueEn":"Neutron stars, formation and structure. \r\nDegenerate neutron gas, equation of state, mass-radius relation. \r\nMass determination in binary systems. \r\nRadio pulsars, X-ray pulsars, accreting millisecond pulsars. \r\nX-ray sources in the Milky Way. Low- and high-mass X-ray binaries. \r\nStellar-mass black holes. Intermediate-mass black holes. \r\nSupermassive black holes in the Milky Way and in other galaxies. \r\nPhysics of accretion, spherical accretion, accretion disks. \r\nObservations of accreting neutron stars and black holes, spectral and temporal properties. \r\nClusters of galaxies. \r\nRelativistic jets in AGN and gamma-ray bursts. \r\nThe course contains a number of demanding computer exercises.","valueSv":""}},{"title":{"valueFi":"Suoritustavat","valueEn":"Study methods","valueSv":""},"content":{"valueFi":"","valueEn":"Participation in classroom work\r\nWritten exam\r\nPresentation, minimum 50% of exercises, and the final exam.","valueSv":""}},{"title":{"valueFi":"Toteutustavat","valueEn":"Course unit methods","valueSv":""},"content":{"valueFi":"","valueEn":"Lectures 40 h \r\nExercises 16 h\r\nHomework, presentation","valueSv":""}},{"title":{"valueFi":"Oppimateriaalit","valueEn":"Learning material","valueSv":""},"content":{"valueFi":"","valueEn":"","valueSv":""}},{"title":{"valueFi":"Lisätiedot","valueEn":"Further information","valueSv":""},"content":{"valueFi":"","valueEn":"Course will be given every other autumn (in even years).","valueSv":""}},{"title":{"valueFi":"Kurssikirjallisuus","valueEn":"Literature","valueSv":""},"content":{"valueFi":"1. Accretion power in astrophysics, by J. Frank, A. King, D. Raine 978-0521629577","valueEn":"1. Accretion power in astrophysics, by J. Frank, A. King, D. Raine 978-0521629577","valueSv":"1. Accretion power in astrophysics, by J. Frank, A. King, D. Raine 978-0521629577"}},{"title":{"valueFi":"Esitietovaatimukset","valueEn":"Qualifications","valueSv":""},"content":{"valueFi":"","valueEn":"Recommended preceding studies: Thermodynamics, Nuclear and Particle Physics, and Theoretical Astrophysics","valueSv":""}},{"title":{"valueFi":"Arviointiasteikko","valueEn":"Assessment scale","valueSv":""},"content":{"valueFi":"0-5","valueEn":"0-5","valueSv":"0-5"}},{"title":{"valueFi":"Arviointikriteerit","valueEn":"Assessment criteria","valueSv":""},"content":{"valueFi":"","valueEn":"","valueSv":""}},{"title":{"valueFi":"Arviointikriteerit 2","valueEn":"Assessment criteria 2","valueSv":""},"content":{"valueFi":"","valueEn":"","valueSv":""}},{"title":{"valueFi":"Arviointikriteerit 3","valueEn":"Assessment criteria 3","valueSv":""},"content":{"valueFi":"","valueEn":"","valueSv":""}},{"title":{"valueFi":"Arviointikriteerit 4","valueEn":"Assessment criteria 4","valueSv":""},"content":{"valueFi":"","valueEn":"","valueSv":""}},{"title":{"valueFi":"Kielet","valueEn":"Languages","valueSv":""},"content":{"valueFi":"englanti","valueEn":"English","valueSv":"engelska"}},{"title":{"valueFi":"Taso","valueEn":"Level","valueSv":""},"content":{"valueFi":"Syventävät opinnot","valueEn":"Advanced Studies","valueSv":""}},{"title":{"valueFi":"Oppiaine","valueEn":"Subject","valueSv":""},"content":{"valueFi":"Tähtitiede","valueEn":"Astronomy","valueSv":"Astronomy"}},{"title":{"valueFi":"Vastuuhenkilöt","valueEn":"Person in charge","valueSv":""},"content":{"valueFi":"Juri Poutanen","valueEn":"Juri Poutanen","valueSv":"Juri Poutanen"}},{"title":{"valueFi":"Luokittelu","valueEn":"Classification","valueSv":""},"content":{"valueFi":"","valueEn":"","valueSv":""}},{"title":{"valueFi":"Linkit","valueEn":"Links","valueSv":""},"content":{"valueFi":"","valueEn":"","valueSv":""}}]}