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Concentrated solar thermal power (CSP) offers a clean renewable source of energy. Combined with energy storage, CSP can be dispatchable, on-demand power, decoupling solar energy supply with consumer energy demand, which is currently difficult with other renewables. Current thermal energy storage methods such as sensible or latent heat are currently cost-prohibitive due to low energy density. Thermochemical energy storage offers a potentially game-changing approach to storage thermal energy in the form of chemical bonds for later release. Thermochemical storage can be orders of magnitude more energy dense than previously explored energy storage methods. Here we explore a reversible decomposition-carbonation reaction involving SrCO3/SrO and CO2.
HPR-20 QIC R&D
The Hiden HPR-20 QIC R&D specialist gas analysis system is a bench-top mass spectrometer for the monitoring of evolved gases and vapors.
For further information on this or other Hiden Analytical products contact Hiden Analytical Inc. at [email protected] or visit the main website at www.HidenInc.com
instruments for advanced science
Solar Thermochemical Energy Storage
SEM image of porous SrO/SrCO3 sample 8
Hiden Analytical Inc. 734.542.6666, 1.888.964.4336 www.HidenInc.com
View Poster on Page 2
A NA L YTICA L
Abstract: Thermochemical energy storage is the next step in creating a self-sustaining society because it allows for energy supply to meet the electricity demand. Chemical bonds provide much higher storage capacities than the conventional energy storage methods; renewable storage schemes with greater energy storage density will potentially have a faster path to economic viability. A potential thermochemical storage cycle lies in the carbonation/decomposition of SrO/SrCO3. It offers the prospect of capturing thermal energy and releasing it at temperatures above 1200°C. One of the fundamental aspects of the project depends on the amount of surface area of the physical structure. To obtain an optimal amount of surface area, the current project involves creating a matrix through the mixing of heat treated SrO and decomposition of sacrificial carbon. The temperatures at which the SrO is being heat treated varied along with the size of the particles being used; also the ratio and size of the carbon particles are being varied to find the optimal structure with the most surface area.
SrCO3 ↔ SrO + CO2(g)
Reversible No catalysis High temperature (~1200°C)Safe
Joanna Julien, Jeremy Grunewald, Kelvin Randhir, Nathan Rhodes, Conrad Cole, Nick AuYeung, Like Li, Renwei Mei, David Hahn
AcknowledgementsWe are very appreciative of funding from Hiden Analytical for participation in this poster session. This work was funded by the U.S. Department of Energy Sunshot Initiative as part of the ELEMENTS program, award DE-EE0006534.
Future Work
Parameter Level Selected Values
A Heat treatment temperature (TH)- 1235 °C+ 1400 °C
B SrO particle size (S) - 25 µm -38 µm+ 106 µm -125 µm
C Graphite particle size (Sg)- 25 µm -38 µm
+ 106 µm – 125 µm
D Mass ratio of graphite to SrO (r) - 0.2+ 0.7
E Structure formation temperature (Ts)- 1100°C+ 1300°C
Preliminary data showing dynamic cycling between 1100 and 1300°C at 10°C/min. pCO2 = 0.33 bar
Ar
Heat Exchanger
Mass Flow Meter
Mass Flow Controllers
High Temperature Furnace
He
CO2
Bed
Pressure transducer
Hiden HPR-20 MS BPR
Investigation into carbonation at elevated pressure
*SEM image of porous SrO/SrCO3 sample 8.
Objective: To find the variable/s that most affects the energy density. It is hypothesized that an optimized amount of surface area will maximize the energy density.
0
500
1000
1500
2000
2500
3000
3500
4000
0 1 2 3 4 5
Ener
gy D
ensi
ty, [
MJ/
m3 ]
Cycle
123456789101112131415-115-21625-38 HT powder106-125 powder20% Polymorphic
Energy Density of Samples
Z-value of the Parameters
*A baseline of 95 percent.
Correlation of results: Lenth’s Method
Procedure:1. A matrix was created
2. Heat treat the SrO
3. Crush and sieve the materials to the appropriate sizes
4. Mix the SrO and graphite to the appropriate ratios
5. Evaluate the reactivity of the samples using a thermo gravimetric analyzer (TGA)
Conclusion: With 5 cycles done with the TGA, the assumption is that the energy density will be stable with continued cycles for each sample. The sample that showed the most promise was sample 15 in terms of energy density. The energy density of 15 started off around 3500 MJ/m^3 in the first cycle and tapered off to just above 1500 MJ/m^3, about 7% higher than the base powder. When comparing the effects of the parameters alone and together, the data shows that both the size of the SrO particles and the graphite particles create a large effect on the energy density. Surface area appears to have an affect on energy density. The next question should be what stabilizes the energy density ?
Solar Thermochemical Energy Storage
Abst
ract
:The
rmoc
hem
ical
ene
rgy
stor
age
is th
e ne
xt st
ep in
cr
eatin
g a
self-
sust
aini
ng so
ciet
y be
caus
e it
allo
ws f
or e
nerg
y su
pply
to m
eet t
he e
lect
ricity
dem
and.
Che
mic
al b
onds
pro
vide
m
uch
high
er st
orag
e ca
paci
ties t
han
the
conv
entio
nal e
nerg
y st
orag
e m
etho
ds; r
enew
able
stor
age
sche
mes
with
gre
ater
ene
rgy
stor
age
dens
ity w
ill p
oten
tially
hav
e a
fast
er p
ath
to e
cono
mic
vi
abili
ty.
A po
tent
ial t
herm
oche
mic
al st
orag
e cy
cle
lies i
n th
e ca
rbon
atio
n/de
com
posit
ion
of S
rO/S
rCO
3. It
offe
rs th
e pr
ospe
ct o
f ca
ptur
ing
ther
mal
ene
rgy
and
rele
asin
g it
at te
mpe
ratu
res a
bove
12
00°C
. O
ne o
f the
fund
amen
tal a
spec
ts o
f the
pro
ject
dep
ends
on
the
amou
nt o
f sur
face
are
a of
the
phys
ical
stru
ctur
e. T
o ob
tain
an
opt
imal
am
ount
of s
urfa
ce a
rea,
the
curr
ent p
roje
ct in
volv
es
crea
ting
a m
atrix
thro
ugh
the
mix
ing
of h
eat t
reat
ed Sr
Oan
d de
com
posit
ion
of sa
crifi
cial
car
bon.
The
tem
pera
ture
s at w
hich
th
e Sr
Ois
bein
g he
at tr
eate
d va
ried
alon
g w
ith th
e siz
e of
the
part
icle
s bei
ng u
sed;
also
the
ratio
and
size
of t
he c
arbo
n pa
rtic
les
are
bein
g va
ried
to fi
nd th
e op
timal
stru
ctur
e w
ith th
e m
ost
surf
ace
area
.
SrCO
3 ↔ S
rO+
CO2(
g)
Re
vers
ible
N
o ca
taly
sis
High
tem
pera
ture
(~12
00°C
)Sa
fe
Joan
na Ju
lien,
Jere
my
Grun
ewal
d, K
elvi
n Ra
ndhi
r, N
atha
n Rh
odes
, Con
rad
Cole
, Nic
k Au
Yeun
g, L
ike
Li, R
enw
ei M
ei, D
avid
Hah
n
Ackn
owle
dgem
ents
We
are
very
app
reci
ativ
e of
fund
ing
from
Hid
en A
naly
tical
for p
artic
ipat
ion
in th
is po
ster
se
ssio
n.
This
wor
k w
as fu
nded
by
the
U.S.
Dep
artm
ent o
f Ene
rgy
Suns
hot I
nitia
tive
as p
art o
f the
EL
EMEN
TS p
rogr
am, a
war
d DE
-EE0
0065
34.
Futu
re W
ork
Para
met
erLe
vel
Sele
cted
Valu
es
AHe
attr
eatm
ent t
empe
ratu
re(T
H)-
1235
°C+
1400
°C
BSr
O p
artic
lesiz
e(S
) -
25 µ
m -3
8 µm
+10
6 µm
-125
µm
CGr
aphi
tepa
rtic
lesiz
e (S
g)-
25 µ
m -3
8 µm
+10
6 µm
–12
5 µm
DM
assr
atio
ofgr
aphi
teto
SrO
(r)
-0.
2+
0.7
ESt
ruct
ure
form
atio
nte
mpe
ratu
re(T
s)-
1100
°C+
1300
°C
Prel
imin
ary
data
show
ing
dyna
mic
cycl
ing
betw
een
1100
and
13
00°C
at 1
0°C/
min
. pC
O2
= 0.
33 b
ar
Ar
Heat
Ex
chan
ger
Mas
s Flo
w
Met
er Mas
s Flo
w C
ontr
olle
rs
High
Te
mpe
ratu
re
Furn
ace
He
CO2
Bed
Pres
sure
tran
sduc
er
Hide
n HP
R-20
MS
BPR
Inve
stig
atio
n in
to c
arbo
natio
n at
ele
vate
d pr
essu
re
*SEM
imag
e of
por
ous S
rO/S
rCO
3 sa
mpl
e 8.
Obj
ectiv
e:To
find
the
varia
ble/
s tha
t mos
t affe
cts t
he
ener
gy d
ensit
y. It
is h
ypot
hesiz
ed th
at a
n op
timize
d am
ount
of
surf
ace
area
will
max
imize
the
ener
gy d
ensit
y.
0
500
1000
1500
2000
2500
3000
3500
4000
01
23
45
Energy Density, [MJ/m3]
Cyc
le
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15-1
15-2
16 25-3
8 H
T po
wde
r
106-
125
pow
der
20%
Pol
ymor
phic
Ener
gy D
ensi
ty o
f Sam
ples
Z-va
lue
of th
e Pa
ram
eter
s
*A b
asel
ine
of 9
5 pe
rcen
t.
Corr
elat
ion
of re
sults
: Len
th’s
Met
hod
Proc
edur
e:1.
A m
atrix
was
cre
ated
2. H
eat t
reat
the
SrO
3. C
rush
and
siev
e th
e m
ater
ials
to th
e ap
prop
riate
size
s
4. M
ix th
e Sr
Oan
d gr
aphi
teto
the
appr
opria
te ra
tios
5. E
valu
ate
the
reac
tivity
of t
he sa
mpl
es u
sing
a th
erm
o gr
avim
etric
ana
lyze
r (TG
A)
Conc
lusi
on:
With
5 c
ycle
s don
e w
ith th
e TG
A, th
e as
sum
ptio
n is
that
the
ener
gy
dens
ity w
ill b
e st
able
with
con
tinue
d cy
cles
for e
ach
sam
ple.
The
sam
ple
that
show
ed th
e m
ost p
rom
ise w
as sa
mpl
e 15
in te
rms o
fen
ergy
de
nsity
. The
ene
rgy
dens
ity o
f 15
star
ted
off a
roun
d 35
00 M
J/m
^3 in
the
first
cyc
le a
nd ta
pere
d of
f to
just
abo
ve 1
500
MJ/
m^3
, abo
ut 7
% h
ighe
r th
an th
e ba
se p
owde
r. W
hen
com
parin
g th
e ef
fect
s of t
he p
aram
eter
s al
one
and
toge
ther
, the
dat
a sh
ows t
hat b
oth
the
size
of th
e Sr
Opa
rtic
les
and
the
grap
hite
par
ticle
s cre
ate
a la
rge
effe
ct o
n th
e en
ergy
den
sity.
Su
rfac
e ar
ea a
ppea
rs to
hav
e an
affe
ct o
n en
ergy
den
sity.
The
nex
t qu
estio
n sh
ould
be
wha
t sta
biliz
es th
e en
ergy
den
sity
?
So
lar
The
rmo
che
mic
al En
erg
y S
tora
ge