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2.4. Solar mediated retro Diels–Alder reaction of 5
3. Results and discussion
The retro Diels–Alder reaction of 5 was carried out using a solar
parabolic dish concentrator with geometrical concentration
ratio of 20 X (Fig. S1†). Experiments were conducted during
11.15 am to 2.15 pm on a typical sunny day in March. Details of
the concentrator and ambient conditions on the day of the
experiment are provided under Section S1 of ESI.† 500 g of 5 was
charged into a 1 L RB ask placed at the focus of the dish. A PV
panel was used to operate a pump to circulate cool water
through a condenser to facilitate condensation of Cp. The
distillate was collected in a 250 mL RB ask placed inside an ice
bag. It was stored in the refrigerator and used as required.
CBS-QB3 method was employed to calculate the changes in DH
and DG of the various reactions considered in the present study.
The data are compiled in Table 1. The method was tested
initially for the formation of quadricyclane from norborna-
diene. The calculated DH of 22.8 kcal molꢀ1 was in good
agreement with the experimental DH value of 21.4 kcal molꢀ1
reported for this process.9 The free energy of reaction was
computed to be 22.7 kcal molꢀ1. The reaction of eqn (4) was
studied next. The computed DH of 23.4 kcal molꢀ1 at 273 K was
again in good agreement with the experimentally determined
value of 21.4 kcal molꢀ1
. Corresponding value of DG was 9.7
15
kcal molꢀ1. The computed DG reduced to 2.0 kcal molꢀ1 at 423
K (Table 1), suggesting that the equilibrium of eqn (4) moves to
the right at higher temperature, in line with the reported
observations. Since the values of DH were similar at 273 K and
423 K, the shi in DG is due to changes in the TDS term in the
free energy equation (DG ¼ DH ꢀ TDS). This term would be
expected to increase with temperature on account of the posi-
tive DS expected from the cracking of one molecule of 5 into two
molecules of Cp.
2.5. Solar mediated synthesis of 1-(3-phenylbicyclo [2.2.1]
hepta-2,5-dien-2-yl) ethanone (7) (see eqn (5))
An offset parabola of concentration ratio 59 X (Fig. S2†) was
employed for the synthesis and the reaction was conducted over
5.5 h (10.00 am to 3.30 pm) on a typical day in March. Details of
the concentrator and ambient conditions on the day of the
experiment are provided in Section S1.† 0.46 g of Cp prepared
above was added along with 1 g of 4-phenylbut-3-yn-2-one (6)
and 15 mL of diphenyl ether (solvent) into a 25 mL single neck
RB ask. The ask was placed at the focal point of the
concentrator which served as source of thermal energy. The
reaction temperature over the reaction period was in the range
of 150–185 ꢁC. Aer termination of the reaction the contents
were charged on a silica gel column and eluted with 5% ethyl
acetate in hexane. 1.1 g (75% isolated yield) of pure 7 was
obtained. 1H NMR (500 MHz, CDCl3) d 7.36–7.35 (d, 2H), 7.33–
7.31 (m, 1H), 7.29–7.28 (d, 2H), 6.98 (s, 1H), 6.88 (s, 1H), 4.09 (s,
1H), 3.77 (s, 1H), 1.99 (s, 3H); 13C NMR (125 MHz, CDCl3) d
196.5, 166.5, 149.4, 143.7, 141.2, 137.0, 128.5, 127.1, 70.3, 59.3,
52.2, 29.1; IR (in KBr, cmꢀ1) 3435, 2931, 2362, 1651, 1443, 1359,
1237, 1022, 759, 699; HRMS (ESI): found 211.1135 (calcd for
Drawing on the kinetics data reported earlier on the retro
Diels–Alder reaction of 5,14 the parabolic dish of Fig. S1† was
designed and fabricated to achieve 175 ꢁC # T # 200 ꢁC under
peak insolation condition (850–1000 W mꢀ2) prevailing in the
summer months in the western part of India. Initially, the
reactor assembly of Fig. S1(A)† was taken, and entries 1 and 2
in Table 2 provide data for experiments conducted on
cracking of 5 on two separate sunny days during March 2014.
The second set of data were taken for further analysis.
Fig. S3(A)† provides data on global insolation, ambient
temperature and temperature in the reaction zone during
10.00 am to 2.00 pm on the day of the experiment pertaining
to entry 2, Table 2. Other weather related data are presented
in Table S1.† The reaction temperature rose gradually from
11.15 am to 12.00 noon and thereaer remained in the range
of 175–190 ꢁC. A thermal image recorded during this period is
shown in Fig. 1. The total volume of Cp collected over 3 h was
154 mL which worked out to an average hourly collection of
51.3 mL hꢀ1 (Table 2). Although hour-wise data were not
collected, the output was highest during 12.30 pm to 1.00 pm.
Based on the collector aperture area (1.83 m2) and average
global insolation (857 W mꢀ2) during the duration of the
experiment, the total energy captured by the parabolic dish
was 1344 kcal hꢀ1. However, the energy available at the
reaction zone was only 5142 kcal hꢀ1 based on pyranometer
reading of the concentrated radiation. This was ascribed to
C
15H14O [M + H], 211.1123).
2.6. Solar mediated synthesis of pentacyclo-
[5.4.0.02,6.03,10.05,9]undecan-8, 11-dione(9) from8 (see eqn (6)).
8 was prepared as a yellow crystalline solid from solar generated
Cp and benzoquinone following literature procedure.22 1 g of 8
was taken in 10 mL of ethyl acetate and placed in a quartz RB
ask positioned at the focus of an 8ꢂ parabolic dish.17a 9 was
obtained as a brown solid (m.p. 240 ꢁC) in 96% yield within 15
min. The reaction temperature was ca. 90 ꢁC. 1H NMR (500
MHz, CDCl3) d 3.18 (s, 2H), 2.94 (s, 2H), 2.82 (d, 2H), 2.71 (s, 2H),
2.06–2.04 (d, 1H), 1.90–1.88 (d, 1H); 13C NMR (125 MHz, CDCl3):
d 212.1, 54.7, 44.6, 43.7, 40.4, 38.7; IR (in KBr, cmꢀ1) 3448, 2990,
2930, 2868, 1753, 1728, 1454, 1267, 1224, 1191, 1056, 966, 911,
860, 823, 755, 600, 525, 453. Observed mass (M + H) 174.96,
calculated mass (M + H) 175.08.
the following reasons: (i) diffuse radiation (ca. 100 W mꢀ2
)
was not concentrated and (ii) there were considerable
reection losses during concentration. Further, in the
experiment as conducted using a glass RB ask, heating
would have been effected mainly by the infrared component
(4500–42 000 nm) in the concentrated radiation. This
component was estimated to be 2424 kcal hꢀ1 based on
measurement of IR intensity in the solar insolation. Taking
Note: safety precautions must be taken while performing
experiments with concentrated solar radiation.
54560 | RSC Adv., 2014, 4, 54558–54564
This journal is © The Royal Society of Chemistry 2014