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Script score query | Reference

Script score query

Uses a script to provide a custom score for returned documents.

The script_score query is useful if, for example, a scoring function is expensive and you only need to calculate the score of a filtered set of documents.

The following script_score query assigns each returned document a score equal to the my-int field value divided by 10.

 GET /_search {
  "query": {
    "script_score": {
      "query": {
        "match": { "message": "elasticsearch" }
      },
      "script": {
        "source": "doc['my-int'].value / 10 "
      }
    }
  }
}
query
(Required, query object) Query used to return documents.
script
(Required, script object) Script used to compute the score of documents returned by the query.

Important

Final relevance scores from the script_score query cannot be negative. To support certain search optimizations, Lucene requires scores be positive or 0.

min_score
(Optional, float) Documents with a score lower than this floating point number are excluded from search results and results collected by aggregations.
boost
(Optional, float) Documents' scores produced by script are multiplied by boost to produce final documents' scores. Defaults to 1.0.

Within a script, you can access the _score variable which represents the current relevance score of a document.

Within a script, you can access the _termStats variable which provides statistical information about the terms used in the child query of the script_score query.

You can use any of the available painless functions in your script. You can also use the following predefined functions to customize scoring:

We suggest using these predefined functions instead of writing your own. These functions take advantage of efficiencies from Elasticsearch' internal mechanisms.

saturation(value,k) = value/(k + value)

"script" : {
    "source" : "saturation(doc['my-int'].value, 1)"
}

sigmoid(value, k, a) = value^a/ (k^a + value^a)

"script" : {
    "source" : "sigmoid(doc['my-int'].value, 2, 1)"
}

random_score function generates scores that are uniformly distributed from 0 up to but not including 1.

randomScore function has the following syntax: randomScore(<seed>, <fieldName>). It has a required parameter - seed as an integer value, and an optional parameter - fieldName as a string value.

"script" : {
    "source" : "randomScore(100, '_seq_no')"
}

If the fieldName parameter is omitted, the internal Lucene document ids will be used as a source of randomness. This is very efficient, but unfortunately not reproducible since documents might be renumbered by merges.

"script" : {
    "source" : "randomScore(100)"
}

Note that documents that are within the same shard and have the same value for field will get the same score, so it is usually desirable to use a field that has unique values for all documents across a shard. A good default choice might be to use the _seq_no field, whose only drawback is that scores will change if the document is updated since update operations also update the value of the _seq_no field.

You can read more about decay functions here.

"script" : {
    "source" : "decayNumericLinear(params.origin, params.scale, params.offset, params.decay, doc['dval'].value)",
    "params": {
        "origin": 20,
        "scale": 10,
        "decay" : 0.5,
        "offset" : 0
    }
}
  1. Using params allows to compile the script only once, even if params change.
"script" : {
    "source" : "decayGeoExp(params.origin, params.scale, params.offset, params.decay, doc['location'].value)",
    "params": {
        "origin": "40, -70.12",
        "scale": "200km",
        "offset": "0km",
        "decay" : 0.2
    }
}
"script" : {
    "source" : "decayDateGauss(params.origin, params.scale, params.offset, params.decay, doc['date'].value)",
    "params": {
        "origin": "2008-01-01T01:00:00Z",
        "scale": "1h",
        "offset" : "0",
        "decay" : 0.5
    }
}

Note

Decay functions on dates are limited to dates in the default format and default time zone. Also calculations with now are not supported.

Functions for vector fields are accessible through script_score query.

Script score queries will not be executed if search.allow_expensive_queries is set to false.

The script_score query calculates the score for every matching document, or hit. There are faster alternative query types that can efficiently skip non-competitive hits:

We recommend using the script_score query instead of function_score query for the simplicity of the script_score query.

You can implement the following functions of the function_score query using the script_score query:

What you used in script_score of the Function Score query, you can copy into the Script Score query. No changes here.

weight function can be implemented in the Script Score query through the following script:

"script" : {
    "source" : "params.weight * _score",
    "params": {
        "weight": 2
    }
}

Use randomScore function as described in random score function.

field_value_factor function can be easily implemented through script:

"script" : {
    "source" : "Math.log10(doc['field'].value * params.factor)",
    "params" : {
        "factor" : 5
    }
}

For checking if a document has a missing value, you can use doc['field'].size() == 0. For example, this script will use a value 1 if a document doesn’t have a field field:

"script" : {
    "source" : "Math.log10((doc['field'].size() == 0 ? 1 : doc['field'].value()) * params.factor)",
    "params" : {
        "factor" : 5
    }
}

This table lists how field_value_factor modifiers can be implemented through a script:

Modifier Implementation in Script Score none - log Math.log10(doc['f'].value) log1p Math.log10(doc['f'].value + 1) log2p Math.log10(doc['f'].value + 2) ln Math.log(doc['f'].value) ln1p Math.log(doc['f'].value + 1) ln2p Math.log(doc['f'].value + 2) square Math.pow(doc['f'].value, 2) sqrt Math.sqrt(doc['f'].value) reciprocal 1.0 / doc['f'].value

The script_score query has equivalent decay functions that can be used in scripts.

Note

During vector functions' calculation, all matched documents are linearly scanned. Thus, expect the query time grow linearly with the number of matched documents. For this reason, we recommend to limit the number of matched documents with a query parameter.

This is the list of available vector functions and vector access methods:

  1. cosineSimilarity – calculates cosine similarity
  2. dotProduct – calculates dot product
  3. l1norm – calculates L1 distance
  4. hamming – calculates Hamming distance
  5. l2norm - calculates L2 distance
  6. doc[<field>].vectorValue – returns a vector’s value as an array of floats
  7. doc[<field>].magnitude – returns a vector’s magnitude

Note

The cosineSimilarity function is not supported for bit vectors.

Note

The recommended way to access dense vectors is through the cosineSimilarity, dotProduct, l1norm or l2norm functions. Please note however, that you should call these functions only once per script. For example, don’t use these functions in a loop to calculate the similarity between a document vector and multiple other vectors. If you need that functionality, reimplement these functions yourself by accessing vector values directly.

Let’s create an index with a dense_vector mapping and index a couple of documents into it.

 PUT my-index-000001 {
  "mappings": {
    "properties": {
      "my_dense_vector": {
        "type": "dense_vector",
        "index": false,
        "dims": 3
      },
      "my_byte_dense_vector": {
        "type": "dense_vector",
        "index": false,
        "dims": 3,
        "element_type": "byte"
      },
      "status" : {
        "type" : "keyword"
      }
    }
  }
}

PUT my-index-000001/_doc/1
{
  "my_dense_vector": [0.5, 10, 6],
  "my_byte_dense_vector": [0, 10, 6],
  "status" : "published"
}

PUT my-index-000001/_doc/2
{
  "my_dense_vector": [-0.5, 10, 10],
  "my_byte_dense_vector": [0, 10, 10],
  "status" : "published"
}

POST my-index-000001/_refresh

The cosineSimilarity function calculates the measure of cosine similarity between a given query vector and document vectors.

 GET my-index-000001/_search {
  "query": {
    "script_score": {
      "query" : {
        "bool" : {
          "filter" : {
            "term" : {
              "status" : "published"
            }
          }
        }
      },
      "script": {
        "source": "cosineSimilarity(params.query_vector, 'my_dense_vector') + 1.0",
        "params": {
          "query_vector": [4, 3.4, -0.2]
        }
      }
    }
  }
}
  1. To restrict the number of documents on which script score calculation is applied, provide a filter.
  2. The script adds 1.0 to the cosine similarity to prevent the score from being negative.
  3. To take advantage of the script optimizations, provide a query vector as a script parameter.

Note

If a document’s dense vector field has a number of dimensions different from the query’s vector, an error will be thrown.

The dotProduct function calculates the measure of dot product between a given query vector and document vectors.

 GET my-index-000001/_search {
  "query": {
    "script_score": {
      "query" : {
        "bool" : {
          "filter" : {
            "term" : {
              "status" : "published"
            }
          }
        }
      },
      "script": {
        "source": """
          double value = dotProduct(params.query_vector, 'my_dense_vector');
          return sigmoid(1, Math.E, -value);
        """,
        "params": {
          "query_vector": [4, 3.4, -0.2]
        }
      }
    }
  }
}
  1. Using the standard sigmoid function prevents scores from being negative.

The l1norm function calculates L1 distance (Manhattan distance) between a given query vector and document vectors.

 GET my-index-000001/_search {
  "query": {
    "script_score": {
      "query" : {
        "bool" : {
          "filter" : {
            "term" : {
              "status" : "published"
            }
          }
        }
      },
      "script": {
        "source": "1 / (1 + l1norm(params.queryVector, 'my_dense_vector'))",
        "params": {
          "queryVector": [4, 3.4, -0.2]
        }
      }
    }
  }
}
  1. Unlike cosineSimilarity that represent similarity, l1norm and l2norm shown below represent distances or differences. This means, that the more similar the vectors are, the lower the scores will be that are produced by the l1norm and l2norm functions. Thus, as we need more similar vectors to score higher, we reversed the output from l1norm and l2norm. Also, to avoid division by 0 when a document vector matches the query exactly, we added 1 in the denominator.

The hamming function calculates Hamming distance between a given query vector and document vectors. It is only available for byte and bit vectors.

 GET my-index-000001/_search {
  "query": {
    "script_score": {
      "query" : {
        "bool" : {
          "filter" : {
            "term" : {
              "status" : "published"
            }
          }
        }
      },
      "script": {
        "source": "(24 - hamming(params.queryVector, 'my_byte_dense_vector')) / 24",
        "params": {
          "queryVector": [4, 3, 0]
        }
      }
    }
  }
}
  1. Calculate the Hamming distance and normalize it by the bits to get a score between 0 and 1.

The l2norm function calculates L2 distance (Euclidean distance) between a given query vector and document vectors.

 GET my-index-000001/_search {
  "query": {
    "script_score": {
      "query" : {
        "bool" : {
          "filter" : {
            "term" : {
              "status" : "published"
            }
          }
        }
      },
      "script": {
        "source": "1 / (1 + l2norm(params.queryVector, 'my_dense_vector'))",
        "params": {
          "queryVector": [4, 3.4, -0.2]
        }
      }
    }
  }
}

If a document doesn’t have a value for a vector field on which a vector function is executed, an error will be thrown.

You can check if a document has a value for the field my_vector with doc['my_vector'].size() == 0. Your overall script can look like this:

"source": "doc['my_vector'].size() == 0 ? 0 : cosineSimilarity(params.queryVector, 'my_vector')"

You can access vector values directly through the following functions:

Note

For bit vectors, it does return a float[], where each element represents 8 bits.

Note

For bit vectors, this is just the square root of the sum of 1 bits.

For example, the script below implements a cosine similarity using these two functions:

 GET my-index-000001/_search {
  "query": {
    "script_score": {
      "query" : {
        "bool" : {
          "filter" : {
            "term" : {
              "status" : "published"
            }
          }
        }
      },
      "script": {
        "source": """
          float[] v = doc['my_dense_vector'].vectorValue;
          float vm = doc['my_dense_vector'].magnitude;
          float dotProduct = 0;
          for (int i = 0; i < v.length; i++) {
            dotProduct += v[i] * params.queryVector[i];
          }
          return dotProduct / (vm * (float) params.queryVectorMag);
        """,
        "params": {
          "queryVector": [4, 3.4, -0.2],
          "queryVectorMag": 5.25357
        }
      }
    }
  }
}

When using bit vectors, not all the vector functions are available. The supported functions are:

Note

When comparing floats and bytes with bit vectors, the bit vector is treated as a mask in big-endian order. For example, if the bit vector is 10100001 (e.g. the single byte value 161) and its compared with array of values [1, 2, 3, 4, 5, 6, 7, 8] the dotProduct will be 1 + 3 + 8 = 16.

Here is an example of using dot-product with bit vectors.

 PUT my-index-bit-vectors {
  "mappings": {
    "properties": {
      "my_dense_vector": {
        "type": "dense_vector",
        "index": false,
        "element_type": "bit",
        "dims": 40
      }
    }
  }
}

PUT my-index-bit-vectors/_doc/1
{
  "my_dense_vector": [8, 5, -15, 1, -7]
}

PUT my-index-bit-vectors/_doc/2
{
  "my_dense_vector": [-1, 115, -3, 4, -128]
}

PUT my-index-bit-vectors/_doc/3
{
  "my_dense_vector": [2, 18, -5, 0, -124]
}

POST my-index-bit-vectors/_refresh
  1. The number of dimensions or bits for the bit vector.
  2. This vector represents 5 bytes, or 5 * 8 = 40 bits, which equals the configured dimensions
 GET my-index-bit-vectors/_search {
  "query": {
    "script_score": {
      "query" : {
        "match_all": {}
      },
      "script": {
        "source": "dotProduct(params.query_vector, 'my_dense_vector')",
        "params": {
          "query_vector": [8, 5, -15, 1, -7]
        }
      }
    }
  }
}
  1. This vector is 40 bits, and thus will compute a bitwise & operation with the stored vectors.
 GET my-index-bit-vectors/_search {
  "query": {
    "script_score": {
      "query" : {
        "match_all": {}
      },
      "script": {
        "source": "dotProduct(params.query_vector, 'my_dense_vector')",
        "params": {
          "query_vector": [0.23, 1.45, 3.67, 4.89, -0.56, 2.34, 3.21, 1.78, -2.45, 0.98, -0.12, 3.45, 4.56, 2.78, 1.23, 0.67, 3.89, 4.12, -2.34, 1.56, 0.78, 3.21, 4.12, 2.45, -1.67, 0.34, -3.45, 4.56, -2.78, 1.23, -0.67, 3.89, -4.34, 2.12, -1.56, 0.78, -3.21, 4.45, 2.12, 1.67]
        }
      }
    }
  }
}
  1. This vector is 40 individual dimensions, and thus will sum the floating point values using the stored bit vector as a mask.

Currently, the cosineSimilarity function is not supported for bit vectors.

Using an explain request provides an explanation of how the parts of a score were computed. The script_score query can add its own explanation by setting the explanation parameter:

 GET /my-index-000001/_explain/0 {
  "query": {
    "script_score": {
      "query": {
        "match": { "message": "elasticsearch" }
      },
      "script": {
        "source": """
          long count = doc['count'].value;
          double normalizedCount = count / 10;
          if (explanation != null) {
            explanation.set('normalized count = count / 10 = ' + count + ' / 10 = ' + normalizedCount);
          }
          return normalizedCount;
        """
      }
    }
  }
}

Note that the explanation will be null when using in a normal _search request, so having a conditional guard is best practice.


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