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Ranking
NSS-CODAS - Neutrosophic Spherical extension of CODAS
Neutrosophic Spherical Set (NSS) outranking - T,I,F ∈ [0,1] independent with squared-norm bound 0 ≤ T²+I²+F² ≤ √3 (Bhuvaneshwari-Sweety 2024 Eq.(2)); combined with CODAS Euclidean-distance ranking
Bhuvaneshwari, S., Antony Crispin Sweety, C.2024
Overview
NSS-CODAS fuses neutrosophic logic (T, I, F triples) with spherical-style squared-norm membership (0 ≤ T²+I²+F² ≤ 3) and applies CODAS-style closeness ratio ranking. Group judgements are pre-aggregated via SWAM or SWGM (Eqs.13-14). Criteria weights are NSS triples aggregated the same way. The revised closeness ratio ξ_i (Eq.28) is interpreted with lower-is-better - opposite to crisp CODAS - because the modification subtracts the NIS-normalised distance from the PIS-normalised distance.
- Output
- utility, lower is better
- Data
- Neutrosophic Spherical, uncertainty tuples complete
- Weights
- Needs a weight source
- Size
- 2+ alternatives, 3-10 criteria works best
- Used for
- Neutrosophic Soft Set MCDM, MAGDM under epistemic uncertainty, expert-driven evaluation with linguistic terms
How it works
- 1
Decision-makers express judgements using NSS linguistic terms (Table 1 of seminal: PMS, ES, HP, RGS, EI, VMS, LP, ELS, DNI), each mapped to a (T, I, F) triple.
Bhuvaneshwari & Antony Crispin Sweety 2024 §4 Step 1; Table 1
- 2
Aggregate decision-maker assessments via SWAM (Eq.13) or SWGM (Eq.14) using DM weights z to produce a single NS decision matrix D = [K_j(S_i)]_{m×n}.
Bhuvaneshwari & Antony Crispin Sweety 2024 Eqs.(13)-(14); §4 Step 2
- 3
Build the weighted aggregated NS decision matrix by NSS multiplication (Eq.4): K_j(S_iz) = ⟨T_ij·T_zj, I_ij·I_zj, F_ij·F_zj⟩ where z = (T_zj, I_zj, F_zj) is the aggregated criterion-weight triple.
Bhuvaneshwari & Antony Crispin Sweety 2024 Eq.(4); §4 Step 3 Eq.(19)
- 4
De-neutrosophise the weighted NS matrix via the score function S(K_j(S_iz)) = (T_ijz − F_ijz)² − (I_ijz − F_ijz)² (Eq.15 / Eq.20).
Bhuvaneshwari & Antony Crispin Sweety 2024 Eq.(15); §4 Step 4 Eq.(20)
- 5
Identify NS-PIS S* (per-criterion arg-max of score) and NS-NIS S^- (per-criterion arg-min of score).
Bhuvaneshwari & Antony Crispin Sweety 2024 Eqs.(21)-(22); §4 Step 5
- 6
Compute Euclidean-type distances from each alternative to NS-PIS and NS-NIS using the NSS spherical distance metric.
Bhuvaneshwari & Antony Crispin Sweety 2024 Eqs.(23)-(24); §4 Step 6
- 7
Compute the per-alternative max distance to NS-NIS (Dmax) and min distance to NS-PIS (Dmin).
Bhuvaneshwari & Antony Crispin Sweety 2024 Eqs.(25)-(26); §4 Step 7
- 8
Compute the revised closeness ratio ξ_i (Eq.28). Lower ξ_i = better alternative.
Bhuvaneshwari & Antony Crispin Sweety 2024 Eq.(28); §4 Step 8
- 9
Rank alternatives in ascending order of ξ_i (lower closeness ratio = better alternative).
Bhuvaneshwari & Antony Crispin Sweety 2024 §4 Step 9
Fits when / Look elsewhere when
Fits when
- •Preserves neutrosophic uncertainty through the pipeline rather than premature crispification at elicitation
- •Native group-decision support (multi-DM aggregation built into the pipeline)
Look elsewhere when
- •Crisp data sufficient - use base CODAS directly (avoid unnecessary uncertainty layer)
- •Aggregation operator (PFWA/PFOWA/etc.) not specified - output ambiguous
Assumptions to verify
- Decision matrix entries are valid Neutrosophic Soft Set numbers/tuples
- Underlying crisp method's compensation assumption holds in uncertain space
- All decision-maker(s) and experts use the same linguistic/uncertainty scale
Edge cases and pitfalls
NSS norm constraint is T²+I²+F² ≤ √3 (NOT ≤ 1 as in spherical fuzzy and NOT linear T+I+F ≤ 3 as in classical neutrosophic). Validate at input.
Ranking direction is inverted vs. crisp CODAS: lower ξ_i = better. Failing to invert misranks all alternatives.
Criterion weights here are NSS triples (T_z, I_z, F_z), not scalars; multiply via NSS multiplication Eq.(4), not scalar multiplication.
Seminal Tables 17 (SWAM closeness values) and the in-text comparison chart show divergent magnitudes (12438 vs 4.146 for S2). The chart values match the SWGM table format; we adopt the chart values as the canonical numeric reference.
Works with
Commonly takes its weights from
How to cite
Bhuvaneshwari, S.; Antony Crispin Sweety, C. (2024). Neutrosophic Spherical Sets in MCDM. Neutrosophic Sets and Systems.
System ID, as it appears in reports and the API
NSS-CODAS