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Theory and Modern Applications

Table 3 (Example 6.1) Comparing \(E^{\mathrm{Re}}_{\infty }(h,\tau )\) and \(E^{\mathrm{Im}}_{\infty }(h,\tau )\) with other methods

From: Quintic non-polynomial spline for time-fractional nonlinear Schrödinger equation

γ

h

\(E^{\text{Re}}_{\infty }(h,\tau )\)

\(E^{\text{Re}}_{\infty }(h,\tau )\)

\(E^{\text{Re}}_{\infty }(h,\tau )\)

\(E^{\text{Im}}_{\infty }(h,\tau )\)

\(E^{\text{Im}}_{\infty }(h,\tau )\)

\(E^{\text{Im}}_{\infty }(h,\tau )\)

Our method

MC [47]

CNS [36]

Our method

MC [47]

CNS [36]

0.1

1/9

1.2703e−04

7.0404e−02

1.2683e−03

1.2556e−04

7.6325e−02

2.4250e−03

1/14

3.0566e−06

2.1873e−02

2.2077e−04

1.0443e−05

2.6090e−02

4.1972e−04

1/19

4.1062e−07

1.0022e−02

6.5147e−05

1.4591e−06

1.2230e−02

1.2268e−04

1/24

9.4755e−08

5.1958e−03

2.5400e−05

3.2571e−07

6.4207e−03

4.8343e−05

1/29

6.5541e−08

2.8536e−03

1.1938e−05

1.0337e−07

3.5662e−03

2.2621e−05

0.3

1/9

1.2838e−04

7.0520e−02

1.3135e−03

1.2426e−04

3.5128e−02

2.3999e−03

1/14

3.1059e−06

2.1979e−02

2.2990e−04

1.0361e−05

1.4733e−02

4.1516e−04

1/19

4.0294e−07

1.0068e−02

6.7510e−05

1.5206e−06

7.1997e−03

1.2140e−04

1/24

4.1570e−07

5.2146e−03

2.6167e−05

4.6692e−07

3.8478e−03

4.7855e−05

1/29

4.3146e−07

2.8610e−03

1.2195e−05

2.9081e−07

2.1771e−03

2.2402e−05