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17 | 17 | import numpy as np
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18 | 18 | from scipy import constants
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19 | 19 | from scipy.constants import physical_constants, speed_of_light
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20 |
| -from scipy.integrate import simps |
| 20 | + |
| 21 | +try: |
| 22 | + from scipy.integrate import simpson |
| 23 | +except ImportError: |
| 24 | + from scipy.integrate import simps as simpson |
21 | 25 | from scipy.interpolate import interp1d
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22 | 26 |
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23 | 27 | from pymatgen.io.vasp.outputs import Vasprun
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@@ -187,7 +191,7 @@ def slme(
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187 | 191 | solar_spectra_photon_flux = solar_spectra_irradiance * (solar_spectra_wavelength_meters / (h * c))
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188 | 192 |
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189 | 193 | # Calculation of total solar power incoming
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190 |
| - power_in = simps(solar_spectra_irradiance, solar_spectra_wavelength) |
| 194 | + power_in = simpson(solar_spectra_irradiance, solar_spectra_wavelength) |
191 | 195 |
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192 | 196 | # calculation of blackbody irradiance spectra
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193 | 197 | # units of W/(m**3), different than solar_spectra_irradiance!!! (This
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@@ -232,15 +236,15 @@ def slme(
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232 | 236 | J_0_r = (
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233 | 237 | e
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234 | 238 | * np.pi
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235 |
| - * simps( |
| 239 | + * simpson( |
236 | 240 | blackbody_photon_flux * absorbed_by_wavelength,
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237 | 241 | solar_spectra_wavelength_meters,
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238 | 242 | )
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239 | 243 | )
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240 | 244 |
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241 | 245 | J_0 = J_0_r / fr
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242 | 246 |
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243 |
| - J_sc = e * simps(solar_spectra_photon_flux * absorbed_by_wavelength, solar_spectra_wavelength) |
| 247 | + J_sc = e * simpson(solar_spectra_photon_flux * absorbed_by_wavelength, solar_spectra_wavelength) |
244 | 248 |
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245 | 249 | def J(V):
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246 | 250 | return J_sc - J_0 * (np.exp(e * V / (k * temperature)) - 1.0)
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