Issue 51
G. Cocchetti et alii, Frattura ed Integrità Strutturale, 51 (2020) 356-375; DOI: 10.3221/IGF-ESIS.51.26
self-weight distribution along the arch ( CCR
= 1, M
= 1), respectively leading to a “linear” , a “quadratic” and a
“cubic problem” in the algebraic solution for unknown triplet A ( ), ( ), h ( described and discussed in [6]. All what will be considered in the following will stick to classical hypothesis M = 0, i.e. by assuming a self-weight distribution along the geometrical centreline of the arch, in classical Heyman sense, though with correct evaluation CCR = 1 of the tangency condition in Eqn. (1) c . An extensive discussion on the differences between the three arising solutions has been reported in [6], including about the spreading discrepancies appearing for over-complete (horseshoe) circular masonry arches. Known Heyman “linear” solution may finally be obtained from Eqns. (1), for CCR = 0, M = 0, and can be classically represented as: ). This is originally and extensively derived,
2
2 2 cos sin cos +
+
sin
=
=
A
cot
cot
2
2 cos sin cos +
−
sin cos
(
)(
)
−
sin 1 cos −
(3)
= =
2
H
(
)
1 cos +
H = = h h
cot
Going to properly correct CCR solution ( CCR = 0), for the complete semi-circular arch, i.e. = A = /2, system (1) renders the following characteristic CCR solution triplet for the purely-rotational collapse mode to be recorded: = 1, M
r
=
0.951141 54.4963 , rad =
r
=
=
=
0.107426,
h
0.621772 (
/ 2)
(4)
r
More generally, at variable half-opening angle of the circular masonry arch (thus at variable A = cot ( /2)), the solution of system (1) for CCR = 1, M = 0 can be analytically represented in closed-form as follows [6]:
2
2
2 (2 ) − + − f S g S
f
gS S
=
A g
f = =
( ) ( sin )'
= +
S C
f
2
( ) = = + = + g g S Cf
SC
2
2
g S f −
2 − +
gS S
2 =
with
(5)
+
f
g
= = = =
( ) sin ( ) cos
S S C C
2
2
2 − − + S f gS S
f
h =
2
S
Indeed, triplet A (
), ( ), h ( ) becomes a double-valued function of inner hinge position , coming from the solution of
the following “quadratic problem” [6]:
2
2
(2 ) S g S A fg A g − − + = 2
0
2
) 4( + − − + − = ) 4( ) 0 g g S g f
(
f
(6)
2
2( − − + − = ) S h g f f
2
S h
0
The above three quadratic equations in A , , ( A , h ) and ( A , ). Notice that solutions (5) b
h can be obtained from system (1) by eliminating in turn couples ( , h ), for and h can be obtained from a 2×2 subsystem formed and (5) c
by Eqns. (1) a ) become single-valued at = s = 1.12909 rad = 64.6918°, namely at the value of setting to zero the term under square roots and (1) c , namely those independent on A ( ) in source system (1). Functions A ( ), ( ), h (
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