• Non ci sono risultati.

We want to show that:

N/A
N/A
Protected

Academic year: 2021

Condividi "We want to show that: "

Copied!
2
0
0

Testo completo

(1)

147

APPENDIX C

We want to show that:

, m m s m .

S S

dS dS

φ ξ φ ξ φ ξ

∇ = ∇ ⋅ ∫∫ = − ∫∫ ∇ ⋅ (C.1) In order to do that, it is convenient to choose a Cartesian reference system with the x and y axis belonging to the plane defined by the generic face S of the triangle domain and with the origin in one of the triangle vertex (Fig. C.1).

Figure C.1. Cartesian reference system belonging to the triangle face S.

Noting that with the chosen reference system the RWG basis does not present any z-component, we obtain:

( ) ( )

( ) , ( ) ( ) , ( )

, , , ,

.

, , , , , ,

m m

S

m x m y

S

x y z x y dxdy

x y z x y x y z x y dxdy

x y

φ ξ φ ξ

φ ξ φ ξ

∇ = ∇ ⋅ =

 ∂ + ∂ 

 ∂ ∂ 

 

∫∫

∫∫ (C.2)

By using the definition (2.20), the (C.2) can be written as:

(2)

VECTOR IDENTITY

148

( ) ( )

, , , , , .

2 2

m m

m

m m

S S

l x l x

x y z dxdy x y z dxdy

x A y A

φ ξ φ φ

±

±

±

±

∂ ∂

∇ = ± ±

∂ ∂

∫∫ ∫∫ (C.3)

The first integral in (C.3) can be evaluated analytically as follow (in a similar way we can solve the second one):

( ) ( )

( ) ( )

( )

0

, , , ,

2 2

, , , , ,

2 2

, , 2

C

B

C

bx x

m m

m ax m

S cx d x

m m

m m

ax x S

m S m

l x l x

x y z dxdy x y z dy

x A A

l x l

x y z dy x y z dxdy

A A

x y z l dxdy A

φ φ

φ φ

φ

±

±

±

± ±

− +

± ±

±

 

∂ =  

∂    

 

 

+ − =

 

 

∫∫ ∫

∫ ∫∫

∫∫

(C.4)

since:

( )

( ) ( )

, , 2

.

, , , , 0

2 2

B

B

C C

C C

cx d

m B B

ax m

B B

bx cx d

m C m C

C C

m m

ax ax

C C

x y z l x dy A

ax cx d

l x l x

x y z dy x y z dy

A A

bx cx d

φ

φ φ

− +

±

− +

± ±

= − +

− =

= − +

∫ ∫

(C.5)

For the relation (C.5) and (2.21), the (C.1) becomes:

( )

( ) ( )

( )

, , ,

, , , , .

, , ,

m m

S m

m m

m m

S S

s m s m

S

x y z l dS A

l l

x y z dxdy x y z dxdy

A A

x y z dS

φ ξ φ

φ φ

φ ξ φ ξ

±

+ −

±

+ −

∇ = =

− + =

 ∇ ⋅  = − ∇ ⋅

 

∫∫

∫∫ ∫∫

∫∫

(C.6)

Riferimenti

Documenti correlati

Then we have studied the abundance gradients along the Galactic disk produced by our best cosmological model and their dependence upon several parameters: a threshold in the surface

We allow for discontinuous coefficients and random initial condition and, under suitable assumptions, we prove that in the limit as the number of particles grows to infinity

Solution proposed by Roberto Tauraso, Dipartimento di Matematica, Universit`a di Roma “Tor Vergata”, via della Ricerca Scientifica, 00133 Roma,

Without loss of generality we may assume that A, B, C are complex numbers along the unit circle. |z|

[r]

Let E be the midpoint of AC, and let F be the midpoint

In what follows we seek to trace and reconstruct, through a series of examples running from the early modern Cartesian context through Enlightenment materialism to mid- 19 th

As before, the choice  D 0:5 fits PL better than our 289 models; but, again, we redrew the graphs using the optimal value of  for each 290 turbulence level, and found no