How old is the universe? (part 2)
Watch video of Vanderbilt Professor David A. Weintraub speaking March 30 on “How Old is the Universe?” as part of the Osher Lifelong Learning Institute. David A. Weintraub is professor of astronomy, director of the Communication of Science & Technology program, and director of Undergraduate Studies for Department of Physics & Astronomy at Vanderbilt University.keep reading »
The Americas in the Age of Revolution, 1776-1836 (part 2)
Watch video of Marshall Eakin, professor of history at Vanderbilt University, speaking March 30 on ”The Americas in the Age of Revolution, 1776-1836,” as part of the Osher Lifelong Learning Institute. The revolution that created the United States was only one of many American revolutions. From 1776 to 1836, wars for independence erupted throughout the Americas—from Bostonkeep reading »
Next Steps
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
6 Summary
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
5.4 The scanning tunnelling microscope
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
5.3 Stellar astrophysics
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
5.2 Alpha decay
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
5.1 Overview
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
4.4 Stationary states and tunnelling in one dimension
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
4.3 Stationary states and barrier penetration
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
4.2 Wave packets and tunnelling in one dimension
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
4.1 Overview
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
3.6 Scattering in three dimensions
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
3.5 Scattering from finite square wells and barriers
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
3.4 Probability currents
Scattering is fundamental to almost everything we know about the world, such as why the sky is blue. Tunnelling is entirely quantum-mechanical and gives rise to such phenomena as nuclear fusion in stars. Examples and applications of both these fascinating concepts are investigated in this unit.
3.4 References Brandwood, G., Davison, A. and Slaughter, M. (2004) Licensed to Sell: The History and Heritage of the Public House, London, English Heritage. Wilkinson, A. (2001) Enough Has Been Bulldozed! Save Farnborough, the Cradle of British Aviation, London, SAVE Britain's Heritage. World Heritage List (2005) ‘The criteria for selection’ (Accessed 27 May
3.3 Managing Edinburgh as a heritage site In 1999, Edinburgh World Heritage Trust, a managing body, was established. In 2005, it published the Edinburgh World Heritage Trust Old and New Towns of Edinburgh management plan. This sets out what is significant about the World Heritage site, and outlines the steps for conserving and managing that significance. It lists the key features of the World Heritage site as follows: landscape setting – its topography of hills and valleys, juxtaposition of
3.2 Justification by State Party Read the Justification by State Party on the ICOMOS website (you only need to read the first nine pages which are the pages in English). How does the site meet the U 3.1 Overview In 1995, a large portion of central Edinburgh – the architecturally significant medieval and early Renaissance ‘Old Town’ and the Georgian ‘New Town’ – were included in the World Heritage List. Capital of Scotland since the fifteenth century, Edinburgh's unique character, a result of its particular combination of medieval fortress city and eighteenth-century neoclassical Georgian city, was given as the reason for its World Heritage status. The ‘Justification by St 2.8 References and further reading Ascherson, N. (2002) Stone Voices: The Search for Scotland (revised edn), London, Granta. Basu, P. (2007) Highland Homecomings: Genealogy and Heritage Tourism in the Scottish Diaspora, London, Routledge. Carman, J. and Carman, P. (2006) Bloody Meadows: Investigating Landscapes of Battle, Thrupp, Sutton. Culloden (1964) DVD, Peter Watkins (director), BBC British Film Institute
Activity 1
