Physics Blog Number
1
- April 29, 2011
The Gamow peak
A recent monograph (The Physics of Inertial Fusion,
by Atzeni and Meyer-Ter-Vehn, Oxford 2004) has a nice description of
the physics of fusion (and the Gamow peak) in Chapter 1, "Nuclear
fusion reactions." This chapter is available online: http://fds.oup.com/www.oup.co.uk/pdf/0-19-856264-0.pdf
, but the entire book is well written, and is worthwhile perusing.
For non-resonant reactions, like DD, the convolution
of the cross section (including the Gamow factor) and the velocity
distribution function (assuming a thermal distribution) results in the
Gamow peak:
where eGp
is proportional to kT, and this result is good for temperatures small
compared with the Gamow energy EG.
Tin, Sn
Tin is one of the more interesting materials.
It is the element with the largest number of stable isotopes (ten!),
because its atomic nuimber, Z=50, is one of the "magic numbers" of
nuclear stability. These nuclear magic numbers are 2, 8, 20, 28,
50, 82, 126, ..., which means that Sn-50 and Sn-132 are both "doubly
magic" nuclei, have both a magic number of protons and a magic number
of neutrons.
Steven Chu
Our Secretary of Energy is a workhorse. As the
journal Science states, he works on science "during nights, weekends,
and on planes - after putting in 70-80 hours a week as energy
secretary." In particular, he's recently published the most precise
measurement of gravitational redshift, using "quantum interference of
atoms," available here:
http://www.uam.es/personal_pdi/ciencias/jcuevas/Teaching/Muller-Peters-Chu-Nature2010.pdf