Andrey Varlamov SPIN-CNR, Italy Physicist in the kitchen
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Transcript of Andrey Varlamov SPIN-CNR, Italy Physicist in the kitchen
Andrey Varlamov SPIN-CNR, Italy in collaboration with
Attilio Rigamonti, Giuseppe Balestrino
Physicist in the kitchen: exploring the gastronomic universe
School & Conference on Nanoscience and Quantum Transport Kiev, October, 9, 2016
General formula for the cooking time
Heat flow
D
∂T ρ,τ( )∂τ
=κΔT ρ,τ( ) =κ 1ρ2
∂∂ρ
ρ2∂T ρ,τ( )∂ρ
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1τ
!
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κ[ ]r2!" $%
τ cook = aD2 + b
1. So--‐boiled egg
τ cook = 0.451M2/3 ln 0.76
Tegg −TwaterTyolk −Twater
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Dr. Charles D. H. Williams, a lecturer in physics at University of Exeter :
Mass (pounds)
Cooking time (hours)
6 3 8 3.5
12 4.5 16 5.5 20 6.5 24 7.35
2. The Thanksgiving day turkey secret
τ cook = aM2/3 + b
τ cook3
M 2
3. Physics of Pasta
Het flow and water diffusion
Cooking time: τ = aD2 +b
Heat transfer:
Water diffusion:
∂T∂τ
=κΔT
∂n∂τ
= DΔn
Tipo di pasta Diametro est. D
Diametro int. d
Tempo di cottura sper.
Tempo di cottura teor.
Capellini n.1 1.15 mm -- 3 min 2 min
Spaghettini n. 3
1.45 mm -- 5 min 5.0 min
Spaghetti n. 5
1.75 mm -- 8 min 8.2 min
Vermicelli n. 7 1.90 mm -- 11 min 10.7 min
Vermicelli n. 8 2.05 mm -- 13 min 13.0 min
Bucatini 2.70 mm 1mm 8 min 25 min ?!
a = 3.8 min / mm2 b = - 3 min
Table of cooking times for the different types of cylindrical shape pasta
τ=aD2 +b
The case of bucatini requires the particular treatment. The
correct formula is: τ=a(D-d)2 +b
For bucatini: τ = 8.2 min !
P=ρgh=2σ/rmin
dmin=2 rmin ~ 4σ/ ρgh h=2cm, σ=0.05 N/m
g=9.8 m/s 2
dmin ~ 1mm
Fall down of our simple theory for too thin pasta
Capellini: D = 1.15 mm
τcap = 3.8 [1.15]2 - 3 ≈ 2 min
aDcr2 + b = 0
Dcr = | b | /a ≈ 0.85mm
When the rod is broken, one could expect that the generated elastic waves help to both pieces of rod to relax to equilibrium.
Invece, si verifica che queste onde aumentano lo stress locale, rendendo probabile la rottura della bacchetta anche in altri punti. Ne consegue una frammentazione.
Fast removing of the constrain from the extremity of the half-rod results in generation of the elastic wave:
Simul.mov
Filtration: the Darcy Law
P(T)=Patm+ΔP
}
ΔP = Q η L/(Sρ κ)
η( °C) = 10 -3 Pa s
ΔP∼4·∙104 Pa → T* ~ 110 °C
Q = m/t~200 g/min
L~ 1 cm
P=Patm
→
S~ 10 cm2
κ ~ 10-12
Q =κ ⋅S ⋅ρ ⋅ ΔP
L ⋅η
Ancestors of pizza in ancient Lmes Pharaonic birthdays in Ancient Egypt
Flat cakes with vegetables used to eat in the Near East and pharaonic Egypt
Ancestors of pizza in ancient Rome In Pseudo Virgilio, poem “Il Moretum”, cooking of some kind of a flat cake dressed by olive oil, salt, garlic and spice herbs was described
The facts to think
Pizza Romana 325-‐ 330 0С à 2 min
Pizza Napoletana: 460-‐490 0С .
40 -‐50 à80-‐100 customers In rush Lme 330 0С à 390 0С .
c= 1MΔQΔT
Specific heat capacity:
Heat flow:
Heat flow: a ligle bit of school physics
M is the body mass, ΔQ is the Heat transferred to it, ΔT is the change of its temperature.
q= - ΔQSΔt
-‐ “speed” of temperature change in the space
Heat flow in a cylinder from hot (T0+DT) to cold (T0). NoIce, the temperature decreases from leL to right!
ΔTΔx"
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coefficient of thermal conducLvity
L t( )
ΔQS ⋅ t
= c ⋅ρ ⋅L t( ) ⋅ ΔT
t= κ ΔT
L t( )
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χ= κc ⋅ρ
PropagaLon of the heat front
Heat length
-‐-‐ is the coefficient of the temperature conducLvity
Exact answer is
Wood oven: Dough/firebrick: νDf=0.65
T1=330 0C, T2=20 0C
T1=330 0C, T2=20 0C, T0=280 0C
T1=230 0C, T2=20 0C, T0=208 0C
Electric oven with steel bogom: Dough/steel: νDS=0.1
What temperature in oven would be good for pizza?
Thermal radiaIon
σ = 5.67 ⋅10−8W / K 4 ⋅m2( )
Its intensity, i.е., the amount of radiaLon energy arriving each second to 1сm2 of surface in the oven, is determined by the Stefan-‐Boltzmann law:
is the so-‐called Stefan-‐Boltzmann constant
ELECTRIC OWEN
For the much less heated electric oven (t=230 0C=503 K) the corresponding amount of energy, incident to 1сm2 of pizza surface, is more than twice less:
WOOD OVEN
RadiaLon contribuLon for baking pizza
Here one should noLce, that, in its turn, the pizza also irradiates out a “flow” of the intensity Since the major part of the baking Lme is required for the evaporaLon of water contained in the dough and toppings, we can assume
𝑇pizza= 100℃ = 373 𝐾 , which results in a radiaLon intensity of
104𝑊/𝑚2, i.e., 15% of the obtained radiaLon, the pizza “returns” to the oven.
The amount of heat 1 cm2 of pizza receives per second through its bogom
Total amount of heat 1 cm2 of pizza receives per second
This value is used to heat 1 cm2 of pizza from 20 0C to the boiling temperature of water 100 0C
During the process of baking the perfect pizza we apparently evaporate water from the dough, tomatoes, cheese, and other ingredients. We need to take the required energy for this into account as well. If one assumes that the mass fracLon α (which is water, for Roman pizza α=20%) evaporates from the dough and all topping one gets: