Temperature dependence of 185 nm photochemical water treatment – The photolysis of water

Temperature dependence of 185 nm photochemical water treatment – The photolysis of water

Accepted Manuscript Title: Temperature dependence of 185 nm photochemical water treatment – The photolysis of water Author: Laith Furatian Madjid Mohs...

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Accepted Manuscript Title: Temperature dependence of 185 nm photochemical water treatment – The photolysis of water Author: Laith Furatian Madjid Mohseni PII: DOI: Reference:

S1010-6030(17)31258-3 https://doi.org/doi:10.1016/j.jphotochem.2017.12.030 JPC 11068

To appear in:

Journal of Photochemistry and Photobiology A: Chemistry

Received date: Revised date: Accepted date:

29-8-2017 9-12-2017 20-12-2017

Please cite this article as: Laith Furatian, Madjid Mohseni, Temperature dependence ¨ ¨/>nm photochemical water treatment ndash The photolysis of of 185 (2017), https://doi.org/10.1016/j.jphotochem.2017.12.030 This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain.

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Laith Furatian, Madjid Mohseni

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Department of Chemical and Biological Engineering, University of British Columbia, Vancouver BC, Canada

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Temperature Dependence of 185 nm Photochemical Water Treatment - The Photolysis of Water

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Abstract

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The photochemical treatment of water using 185 nm radiation forms the basis of an

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advanced oxidation process (AOP) that does not require chemical addition. The

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185 nm photolysis of water generates the hydroxyl radical ( ·OH) able to degrade

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trace organic contaminants. However, the strong absorbance of water (αH2 O ) at

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185 nm imposes severe geometrical constraints on reactor design. Investigation of

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the reported temperature dependence of αH2 O on treatment efficiency was conducted

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between 5 and 35 ◦C, in model solutions using carbamazepine as a radical probe.

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Comparison was made with the temperature dependence of the 254 nm photolysis of

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hydrogen peroxide under similar conditions. It was found that the 185 nm AOP is

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less sensitive to temperature under the conditions tested, suggesting the absorbance

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of water has a negligible effect in this range. This is postulated to be due to the

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fundamental structure of liquid water, whereby 185 nm photons are absorbed by a

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small population of interstitial H2 O monomers, with no hydrogen bonds to impede

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the escape of ·OH from the solvent cage.

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Keywords: advanced oxidation, ultraviolet, water photolysis, hydroxyl radical,

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monomer

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Email address: [email protected] (Madjid Mohseni) Preprint submitted to Journal of Photochemistry and Photobiology A

December 4, 2017

Page 1 of 22

1. Introduction

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The conventional low-pressure mercury-vapour discharge lamp generates high inten-

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sity UV radiation primarily at 254 and 185 nm (1). The irradiation of water at 254 nm

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is particularly effective at the inactivation of chlorine resistant protozoan pathogens

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(2; 3), and is now widely employed in drinking water treatment at municipal scale

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(4; 5). In addition to disinfection, 254 nm photolysis of H2 O2 generates the highly re-

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active ·OH, thus constituting an advanced oxidation process (AOP) (6). AOPs may

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be applied to augment drinking water treatment when sources are impaired by trace

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organic chemical contaminants refractory to conventional treatment. The 254 nm

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photolysis of H2 O2 is recognized as one of the most practical AOPs for drinking wa-

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ter treatment, offering a compact footprint, the absence of a waste stream, avoidance

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of bromate formation, and simultaneous disinfection. However, the on-site storage of

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concentrated H2 O2 , its addition upstream of UV reactors, and its subsequent removal

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prior to distribution introduce increased process complexity and cost. The 185 nm

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emission is of approximately five to ten times lower intensity than that of 254 nm (1),

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and is unused by 254 nm-H2 O2 based AOPs. The potential to exploit 185 nm radia-

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tion for photochemical purification of water has been recognized for some time (7; 8).

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The 185 nm wavelength occurs at the start of the broad absorption band of the first

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excited state of water (9), with the decadic absorption coefficient for pure water

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(aH2 O ) of 1.8 cm−1 (10), and resulting in the photolysis of water to generate ·OH

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with a quantum yield (ΦH2 O ) of 0.3 (11):

185 nm

H2 O −−−−→ H· + ·OH

ΦH2 O = 0.3

(1)

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Page 2 of 22

In the presence of dissolved oxygen, H· is scavenged at diffusion limited rates (12),

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to produce the relatively nonreactive acid-base pair HO2· /O2· – (13):

HO2· O2·− + H+

k = 2 × 1010 M−1 s−1

(2)

pKa = 4.8

cr

H· + O2 −→ HO2·

ip t

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(3)

The relatively longer lifetime of ·OH results in oxidative conditions and thus an AOP

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that does not require chemical addition.

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The high absorbance of water at 185 nm imposes substantial geometrical constraints

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on reactor design, with approximately 99% of photons absorbed within a path length

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of 1 cm in natural waters. As the lifetime of photogenerated radicals is on the or-

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der of microseconds (14), substantial mixing is required to ensure treatment of any

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non-irradiated reactor volume. A temperature coefficient for aH2 O of 0.05 cm−1 ◦C−1

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has been reported between 20 and 50 ◦C (10; 15). The behaviour at lower tempera-

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tures is not known. The impact of changes in aH2 O due to temperature depends on

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reactor design. For reactors that minimize the non-irradiatd volume by using short

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optical path lengths (≤ 1 cm), operation at lower temperatures may result in a 5 to

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10% of 185 nm radiation reaching the reactor wall, with a corresponding decrease in

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absorption and treatment efficiency.

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Seasonal fluctuations in surface water temperature may span a range from 0 to 20 ◦C

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or more at latitudes far from the equator. Treatment processes in such locations

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must ensure adequate performance regardless of temperature. While UV disinfec-

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tion is relatively insensitive to water temperature, the influence of temperature on 3

Page 3 of 22

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UV based AOPs is not well documented.

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The temperature dependence of the quantum yield ΦH2 O at 185 nm is not known,

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but may be assumed to follow an Arrhenius type relation with an activation energy

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dependent on competing rates of radical recombination kr and escape ke from the

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solvent cage:

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185 nm

ke · · − * → H· + ·OH H2 O − ) −− −− − − [H , OH]aq −

(4)

an

kr

The effective activation energy EΦ will depend on kr and ke , which were not di-

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rectly accessible experimentally in the current study. The situation is analogous for

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254 nm photolysis of H2 O2 , though more information is available on the tempera-

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ture dependence of the quantum yield ΦH2 O2 , which is approximately unity at 25 ◦C

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(16; 17):

254 nm

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ke · · − * → HO· + ·OH H2 O2 − ) −− −− − − [HO , OH]aq −

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(5)

kr

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Based on the limited data reported in the literature for 254 nm photolysis of H2 O2 ,

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an activation energy EΦ for ΦH2 O2 at 254 nm is estimated to be in the range of 11 to

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13 kJ mol−1 (16; 18; 19).

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The temperature dependence of the 185 nm based AOP is a critical factor for con-

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sideration in efficient 185 nm reactor design and is reported here for the first time.

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A comparison with the temperature dependence of the 254 nm-H2 O2 AOP and fun-

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damental insight into the structure of liquid water are also discussed.

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2. Theory

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The ·OH driven treatment of UV based AOPs involves composite chemical reactions.

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Component steps include photolytic generation of ·OH, reaction with target contam-

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inants, and competition reactions with major solutes that act as radical scavengers.

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These component steps themselves are composed of multiple elementary reactions.

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Despite this complexity, the net reaction rate of many composite reactions may be

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represented by a single Arrhenius expression, involving an overall experimentally

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observed activation energy (20):

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k 0 = Atot e−Etot /RT

(6)

where k 0 is an overall reaction rate constant, Atot is the pre-exponential factor, Etot is

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the activation energy, R is the universal gas constant 8.314 46 J K−1 mol−1 , and T is

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the absolute temperature. Component steps may have individual activation energies.

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Whether ·OH is generated by 185 nm photolysis of H2 O, or 254 nm photolysis of

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H2 O2 , the experimentally observed k 0 for the ·OH degradation of a trace organic

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contaminant C, in a solution containing a much larger concentration of the scavenger

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S, and under steady-state conditions, may be expressed by:

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k0 =

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kOH,C ΦΘ kOH,S

(7)

where kOH,C and kOH,S are the relevant second order ·OH rate constants, Φ is the 5

Page 5 of 22

corresponding quantum yield, and Θ contains all other terms assumed to be tem-

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perature independent. In order for k 0 to remain constant throughout the irradiation,

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the condition kOH,C [C]  kOH,S [S] must be satisfied. Equation 7 may be expanded

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in terms of the three components as:

(10)

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with Etot obtained from the experimental data and:

ln(k 0 ) = ln(Atot Θ) − Etot /RT 107

(9)

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Etot = EC + EΦ − ES 106

(8)

from which the Etot may be related to the component activation energies by:

an

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AC e−EC /RT AΦ e−EΦ /RT Θ AS e−ES /RT

us

k0 =

ip t

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If Θ possesses a significant temperature dependence, then a plot of ln(k 0 ) vs. 1/T

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will reveal curvature. In the case of 185 nm radiation, the term Θ contains aH2 O .

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The absence of such curvature indicates that aH2 O temperature sensitivity is negligi-

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ble under the conditions tested. Furthermore, it allows the estimation of one of the

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component activation energies if the others are known. For diffusion limited reac-

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tions, such as those involving ·OH, E is often in the range of 10 to 20 kJ mol−1 (12).

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Examples of E for ·OH reactions include 21 kJ mol−1 for HCO3 – and 10 kJ mol−1 for

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tert-butanol (12). It is important to note that an activation energy is not necessarily 6

Page 6 of 22

associated with an elementary reaction nor a transient intermediate. Nevertheless,

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the concept may be useful in gaining mechanistic insights.

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3. Methods and Materials

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3.1. Overall Approach

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Experiments consisted of a series of batch irradiations of assembled solutions of

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known composition spiked with a probe compound and held in a temperature con-

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trolled vessel. Under steady-state conditions, degradation of the probe compound C

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follows pseudo-first order kinetics with an experimentally observed rate constant k 0 :

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M

ln([Ct ]/[Co ]) = −k 0 t

(11)

with changes in k 0 correlated to changes in solution temperature using Equations 7

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and 8. All solutions contained approximately 0.25 µM of carbamazepine (CBZ) as the

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probe, and 8 mg L−1 as C (0.2 mM) of tert-butanol as scavenger. For 254 nm-H2 O2

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studies, 3.5 mg L−1 (0.1 mM) of H2 O2 was added prior to irradiation. All exposures

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were performed in triplicate. Bovine catalase was used to quench H2 O2 following

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irradiation. Dark controls for 254 nm-H2 O2 tests were also included.

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3.2. Materials

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Solutions were made using ultrapure water produced by an Elga Purewater Option-Q

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system (Elga Labwater, UK) and analytical grade reagents (Sigma Aldrich, USA).

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The 185 nm optical path in the collimation tube was purged with ultrapure nitrogen

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Page 7 of 22

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(Praxair, Canada).

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3.3. Apparatus

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UV irradiations using conventional low pressure mercury lamps (Light Sources Inc,

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USA) were conducted using two types of quasi-collimated beam apparatus (21). For

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254 nm-H2 O2 experiments, a 42 W lamp was used with a quartz envelope doped

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with titanium to block 185 nm. For experiments using both 185 and 254 nm, a sec-

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ond apparatus was equipped with a 10 W lamp not doped with titanium and thus

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transparent to both wavelengths. The optical path of the 185 nm enabled beam was

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purged with ulatrapure nitrogen gas to prevent ozone formation. Samples exposed

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to 254 nm alone were placed in open vessels with small stir bars and a liquid depth

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of approximately 2.0 cm. Samples exposed to both 185 and 254 nm were sealed in

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cylindrical fused silica cells of 1.0 cm path length (Starna, UK) with miniature teflon

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coated stir bars. The distance from the lamps to liquid surface were made at least

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five times the aperture to ensure quasi-collimation and held fixed for all experiments.

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The 185 nm irradiations used a custom made Peltier temperature controlled cell

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holder (Quantum Northwest, USA). The 254 nm-H2 O2 tests used a custom water

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jacketed borosilicate beaker (Cansci, Canada) with temperature controlled by a re-

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circulating chiller (Thermo Fisher Scientific, USA). In both cases, temperature con-

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trol within ± 0.1 ◦C was verified via fine gage thermocouple (Omega, Canada).

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3.4. Probe Compound Selection and Characterization

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Since typically molar absorption coefficients () are less than 105 M−1 cm−1 and quan-

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tum yields (Φ) are less than unity (22), direct photolysis at 185 nm is generally neg8

Page 8 of 22

ligible for contaminants or probes in aqueous systems at concentrations of 1 µg L−1

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or less. Thus, the two main degradation processes for trace contaminants include

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direct photolysis at 254 nm and oxidation by ·OH generated by 185 nm photolysis of

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water. In order to study the effects of 185 nm alone, a simple method involves se-

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lecting a probe compound for which the rate constant for direct photolysis at 254 nm

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is negligible. In solutions of low absorbance (Aλ < 0.02), the rate of direct pho-

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tolysis at 254 nm (kd0 ) is proportional to the product of molar absorption coefficient

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(254 ) and photolysis quantum yield (Φ254 ) (23). Carbamazepine (CBZ) was found

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to satisfy this condition well, with experimentally determined values 254 and Φ254

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listed in Table 1. While para-chlorobenzoic acid (pCBA) has often been used as

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a probe compound in AOP studies, the use of CBZ eliminates the need to correct

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for direct photolysis at 254 nm under typical fluence values (doses), and its superior

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chromatography by HPLC provide wider dynamic range and a lower limit of quanti-

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tation. The second-order ·OH rate constant for CBZ was determined experimentally

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by competitive kinetics with pCBA as the reference (24).

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Table 1: Photochemical reaction parameters for probe compounds at 254 nm

Compound 254 (M−1 cm−1 ) CBZ pCBA

a

Φ254

kOH,C (M−1 s−1 )

6759 ± 190 0.00067 ± 0.00002 6.8 ± 0.6 × 109 3410 ± 75 0.011 ± 0.003 5.0 × 109 a

Reference (24)

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3.5. Analysis

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CBZ and pCBA were quantified by HPLC using a Dionex UltiMate 3000 System

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(Thermo Fisher Scientific, USA). A 100 µL injection volume was delivered to a mobile 9

Page 9 of 22

phase composed of 30% acetonitrile and 70% water acidified to pH 2.5 with 10 mM

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phosphoric acid, in an isocratic flow of 1.0 mL min−1 though a Nova-Pak C18 column

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(Waters Corp., USA) maintained at 35 ◦C. UV detection was performed using 211

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and 239 nm. The t-butanol concentration was verified by a GE Sievers M9 TOC An-

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alyzer (GE Analytical Instruments, USA), using the UV-persulfate method. Absence

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of anionic impurities was verified by HPLC using a Dionex Ion Chromatography sys-

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tem. Hydrogen peroxide was measured using the I3 – method (25). Fluence rates at

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254 nm, used for determinations of Φ254 , were measured using KI−KIO3 actinometry

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(26; 27). Absorbance measurements for 254 determinations, H2 O2 quantitation, and

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KI−KIO3 actinometry, were made using a Shimadzu UVmini-1240 Spectrophotome-

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ter (Shimadzu, Japan).

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4. Results

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All decay curves exhibit first-order kinetics. Note that all experimental data and

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calculations presented here are available in the associated dissertation (28).

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4.1. 254 nm - H2 O2 Regime

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The results for 254 nm - H2 O2 tests are displayed in Figure 1. The reaction rate

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observed increases with temperature from 5 to 35 ◦C, as expected.

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Page 10 of 22

3.4. Results 0

ip t

5 C

cr

0.4

20 C

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0.6

0.8

an

ln([CBZ]t /[CBZ]o )

0.2

35 C

1

10

20

30

M

0

40

50

60

Time (min)

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3.1: Temperature dependence 254 nm - H2 O [HL2−1 O2. ] [tBuOH] = 2 2 regime. Figure 1:Figure Temperature dependence in 254 nm - Hin ] = 3.5 mg = 2 O2 regime. [H 2O −1 3.5 mg L 1 . [tBuOH] = 8 mg L 1 as C. [CBZ] ' 0.25 µM. 8 mg L as C. [CBZ]o ' 0.25 µM. o

The values of k 0 are calculated from linear regression of the triplicate measurements

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for each irradiation time used, with the standard error of the slope used to express

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uncertainty σk0 . The uncertainty of ln(k 0 ) is calculated from the approximation

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σln(k0 ) ≈ σk0 /k 0 (29). The calculated values are displayed in Table 2.

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Table 2: Effect of temperature on removal rate of CBZ in 254 nm-H2 O2 regime

T (◦C)

k 0 × 103 (min−1 ) ln(k 0 )

5

20

35

7.3 ± 0.3 11.4 ± 0.2 16.1 ± 0.5 −4.92 ± 0.04 −4.47 ± 0.02 −4.13 ± 0.03

[H2 O2 ] = 3.5 mg L−1 , [tBuOH] = 8 mg L−1 as C, [CBZ]o ' 0.25 µM

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Page 11 of 22

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The Arrhenius plot for the 254 nm-H2 O2 regime is displayed in Figure 2 using the

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data tabulated in Table 2 and the linearized Equation 6. 3.4. Results

ip t

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cr

4.2

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ln(k0 )

4.4

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4.6

4.8

5 3.1

3.3

3.4

3.5

M

3.2

1/T ⇥

103

K

3.6

3.7

1

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Figure 2:Figure Arrhenius for 254plots nm-Hfor regime. ] = 3.5 mg [tBuOH] 3.2: plots Arrhenius nm-H[H [H2LO−12]. = 3.5 mg L= 81 .mg L−1 as 2 O2254 2O 2O 2 2regime. 1 C. [CBZ][tBuOH] = 8 mg L as C. [CBZ]o ' 0.25 µM. o ' 0.25 µM.

Temperature E↵ects in the 185 nm Regime 4.2. 1853.4.2 nm Regime

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The results for 185 nm tests are displayed in Figure 3.3. As with the preThe results for 185 nm tests are displayed in Figure 3. As with the previous case,

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vious case, the reaction rate is observed to increase with temperature from

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the reaction is observed to increase with temperature from 5 to 35 ◦C, though 5 C torate 35 C. to a lesser extent. As with the 254 nm-H2O2 regime, the observed pseudo-first order rate constants k 0 are calculated from linear regression of the triplicate measurements for each irradiation time used, with the standard error of the slope used to express uncertainty

k0 .

from the approximation in Table 3.2.

As before, the uncertainty of ln(k 0 ) is calculated

ln(k0 )



k0 /k

0.

The calculated values are displayed

The Arrhenius plot for the 185 nm regime is displayed in Figure 3.4 using the data tabulated in Table 3.2.

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Page 12 of 22

3.4. Results 0

ip t

5 C

cr

2

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20 C

3

35 C

an

ln([CBZ]t /[CBZ]o )

1

0

2

4

M

4

6

8

10

12

Time (min)

te

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3.3: Temperature dependence in 185[tBuOH] nm regime. Figure 3:Figure Temperature dependence in 185 nm regime. = 8 mg[tBuOH] L−1 as C.=[CBZ]o ' 1 as C. [CBZ] ' 0.25 µM. 8 mg L o 0.25 µM. The slopes of both Arrhenius plots, as calculated by linear regression, allow

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The values of k 0 and associated uncertainty are calculated in the same fashion as

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before and displayed in Table 3. and are 254 nm-H 2O2 regimes. The values are displayed in Table 3.3.

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the determination of the experimental activation energy for both the 185 nm

Table 3: Effect of temperature on removal rate of CBZ in 185 nm regime

T (◦C)

k 0 × 102 (min−1 ) ln(k 0 )

5

20

35

24.7 ± 0.2 30.5 ± 0.5 35.6 ± 0.5 −1.40 ± 0.01 −1.19 ± 0.02 −1.03 ± 0.01

[tBuOH] = 8 mg L−1 as C, [CBZ]o ' 0.25 µM

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The Arrhenius plot for the 185 nm regime is displayed in Figure 4 using the data

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tabulated in Table 3.

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Page 13 of 22

Table 3.3: Experimental (overall) activation energies for carbamazepine degradation in the presence of tert-butanol in 254 nm-H2O2 and 185 nm regimes

Ea (kJ mol

1)

254 nm-H2O2

185 nm

18.7 ± 0.9

8.6 ± 0.5

NB: These values pertain to the composite reactions and not elementary steps.

ip t cr

1.2

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ln(k0 )

1

1.4

3.2

3.3

3.4

3.5

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3.1

1/T ⇥

103

K

3.6

3.7

1

1

M

3.4: Arrhenius plotsin for regime.[tBuOH] [tBuOH] 8 mg L as as Figure 4: Figure Temperature dependence 185185 nmnm regime. == 8 mg L−1 C. C. [CBZ]o ' 0.25 µM. [CBZ]o ' 0.25 µM.

The slopes of both Arrhenius plots, as calculated by linear regression, 63 allow the

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determination of the experimental activation energy Etot for both the 185 nm and

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254 nm-H2 O2 regimes and are displayed in Table 4.

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Table 4: Experimental (overall) activation energies for carbamazepine degradation in the presence of tert-butanol in 254 nm-H2 O2 and 185 nm regimes

Ea (kJ mol−1 )

254 nm-H2 O2

185 nm

18.7 ± 0.9

8.6 ± 0.5

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5. Discusion

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The results indicate that the 185 nm AOP is less temperature sensitive than the

215

254 nm-H2 O2 AOP under the conditions tested. This result is understood to apply

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to water matrices for which H2 O is the major absorber of 185 nm photons, where the 14

Page 14 of 22

scavenging term Σki [Si ] has a magnitude greater than 105 s−1 and where the activa-

218

tion energy of the target contaminant is less than the effective activation energy for

219

the scavenging term (i.e. EC < ES ). If the last condition is reversed (i.e. EC > ES ),

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the observed rate k 0 may follow an inverse relationship with temperature.

ip t

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In the present case, the scavenger is the pure substance tert-butanol, with an ·OH

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activation energy ES reported as 10 ± 3 kJ mol−1 (30). Using an average of the

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reported values of the activation energy of H2 O2 photolysis at 254 nm, EΦ = 12 ±

us

cr

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1 kJ mol−1 , allows the estimation of the activation energy of ·OH with CBZ, EC ,

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using equation 9. In this manner, the value EC = 17 ± 5 kJ mol−1 is obtained.

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Application of equation 9 for the 185 nm regime allows for the estimation of EΦ , the

228

activation energy of the 185 nm photolysis of water itself. A value of EΦ ≈ 0 kJ mol−1

229

is obtained. The fundamental activation energies deduced from experimental data

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are listed in Table 5.

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Table 5: Summary of fundamental activation energies estimated from this work ·

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Ea (kJ mol−1 )

185 nm

OH + CBZ

H2 O −−−−→ H· + ·OH

17 ± 5

≈0

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Explanation for the EΦ ≈ 0 kJ mol−1 value of H2 O photolysis at 185 nm relates to

232

the presence of H2 O monomers in the structure of the liquid state. While the pre-

233

cise structure of liquid H2 O remains in dispute (31), the conventional view based

234

on evidence from X-ray and neutron diffraction depicts virtually all molecules of

235

H2 O as dynamically hydrogen bonded to an average of four neighbours in an ice-like

236

tetrahedral motif with distorted bond angles (32; 33). The existence of non-hydrogen

237

bonded interstitial H2 O molecules (monomers) is supported by evidence from Raman

238

and infrared spectroscopy, though the proportion of such molecules is interpreted to 15

Page 15 of 22

239

be small (< 1%).

240

Evidence from far-UV absorption also supports the existence of interstitial H2 O

242

monomers. Extensive measurements of 185 nm absorption of ultrapure water in

243

both the vapour and liquid state have been reported (34), confirming observations

244

by others that the molar absorption coefficient of H2 O vapour is three orders of mag-

245

nitude greater than that of the liquid (10; 15; 35). Values of v = 22.1 M−1 cm−1

246

and ` = 0.0274 M−1 cm−1 at 23.5 ◦C were reported for the vapour and liquid states

247

respectively, with measurements of liquid absorption made at increasing temperature

248

(34). The ratio ` /v remained approximately 0.0012 between 23 and 27 ◦C, rising

249

sharply above 30 ◦C to 0.0090 at 91.8 ◦C. Such observations may be explained by

250

the existence of gas-like monomers in the liquid state, representing a fraction of all

251

molecules on the order of 10−3 in the vicinity of 20 ◦C, and with monomers responsible

252

for virtually all 185 nm photon absorption. The temperature dependence reported

253

by Stevenson is interpreted as an increase in monomer population with temperature

254

that nevertheless remains a minority even near the boiling point. This potentially

255

oversimplified depiction is consistent with the considerable degree of hydrogen bond-

256

ing remaining at the boiling point and the relatively high critical temperature of

257

water (36).

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ip t

241

259

Upon 185 nm excitation of an H2 O monomer, only a relatively weak van der Waals

260

force must be overcome in order for the photo-products to escape the solvent cage,

262

since no hydrogen bonds are involved. Though the excited H2 O molecule may lose √ energy to the solvent by collision with a rate constant kr proportional to T , the

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excess energy of the excited molecules itself is likely sufficient to overcome a van der

264

Waals energy of ∼ 5 kJ mol−1 . The activation energy for the photolysis of an H2 O

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molecule, Eφ ≈ 0, applies to the excited-state molecule that has absorbed a 185 nm photon. Such photons possess an energy of 647 kJ mol−1 while the bond-dissociation

267

energy between HO and H is approximately 494 kJ mol−1 (37). The excess energy, is

268

more than sufficient to overcome a postulated van der Waals force.

269

6. Conclusion

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The temperature studies conducted indicate that, under the conditions tested, the

271

185 nm-AOP is relatively insensitive to temperature, potentially simplifying reactor

272

design. An activation energy for the ·OH reaction with carbamazepine has been

273

estimated as 17 ± 5 kJ mol−1 , which should be compared to the effective activation

274

energy of the background organic matter in kinetic studies when temperature is

275

varied. The activation energy for the 185 nm photolysis of H2 O has been estimated

276

to be approximately 0 kJ mol−1 and supports the view that 185 nm photon absorption

277

occurs in interstitial non-hydrogen bonded H2 O monomers present as an approximate

278

10−3 fraction of all molecules. Additional temperature dependence studies should be

279

investigated in water matrices for which H2 O is not the major absorber of 185 nm

280

photons.

281

Acknowledgements

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The Natural Sciences and Engineering Council of Canada (NSERC) and the RES'EAU-

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WaterNET Strategic Network are acknowledged for financial support of this work.

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