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Graham Slater's 2013 SVP talk
1. TempoorMode in Evolution?
The Case of Mammalian Body
Size Evolution
Graham Slater
Department of Paleobiology, National Museum of Natural
History
www.fourdimensionalbiology.co
m
2. “Unifying Fossils and Phylogenies for
Comparative Analyses of Diversification and
Trait Evolution”
organization
- Luke Harmon*
- Rob Freckleton
- Sam Ponton
authors
- Gene Hunt
- Pete Wagner
- Jon Marcot
- Dave Bapst
- Tom Ezard
- Gavin Thomas
- Andy Purvis
reviews
- Arne Mooers
- Dave Polly
-FolmerBokma
- Graeme Lloyd
data
- Peter Smits
- Greg Wilson
3.
4. How fast do
animals evolve?
That is one of the
fundamental
questions
regarding
evolution.
Simpson (1944,
Photo: Florida Museum of Natural
History
27. phenotype
OU is an equilibrium process
starting state
starting state
σ2 / 2α
rate σ2
rubber band parameter α
time
28. BM and OU simulated at the same rate give
very different disparities
phenotype
Brownian motion
Ornstein-Uhlenbeck
time
29. ln(body mass) disparity
the OU process has an equilibrium
disparity
α= 0.01
2 = 0.97
σ
T
J
Mesozoic
K
Pg
Ng
Cenozoic
30. ln(body mass) disparity
a low BM rate increases disparity
2=
σ
α= 0.01
2 = 0.97
σ
T
J
Mesozoic
K
Pg
0.1
Ng
Cenozoic
31. Do we really think
Variation in the Mode of
theTempoof mammalian
evolution is a more
body size evolution
intuitive and more likely
increased after the K-PG
explanation that variation
extinction?
in Tempo
32. Do we really think the
Tempoof mammalian
body size evolution
increased after the K-PG
extinction?
33. How fast do
animals evolve?
That is one of the
fundamental
questions
regarding
evolution.
Simpson (1944,
Photo: Florida Museum of Natural
History