jiwonyou0420/encoder-qa-finetuned

SentenceTransformer based on jiwonyou0420/MNLP_M2_document_encoder

This is a sentence-transformers model finetuned from jiwonyou0420/MNLP_M2_document_encoder. It maps sentences & paragraphs to a 384-dimensional dense vector space and can be used for semantic textual similarity, semantic search, paraphrase mining, text classification, clustering, and more.

Model Details

Model Description

• Model Type: Sentence Transformer
• Base model: jiwonyou0420/MNLP_M2_document_encoder
• Maximum Sequence Length: 512 tokens
• Output Dimensionality: 384 dimensions
• Similarity Function: Cosine Similarity

Model Sources

• Documentation: Sentence Transformers Documentation
• Repository: Sentence Transformers on GitHub
• Hugging Face: Sentence Transformers on Hugging Face

Full Model Architecture

SentenceTransformer(
  (0): Transformer({'max_seq_length': 512, 'do_lower_case': True}) with Transformer model: BertModel 
  (1): Pooling({'word_embedding_dimension': 384, 'pooling_mode_cls_token': True, 'pooling_mode_mean_tokens': False, 'pooling_mode_max_tokens': False, 'pooling_mode_mean_sqrt_len_tokens': False, 'pooling_mode_weightedmean_tokens': False, 'pooling_mode_lasttoken': False, 'include_prompt': True})
  (2): Normalize()
)

Usage

Direct Usage (Sentence Transformers)

First install the Sentence Transformers library:

pip install -U sentence-transformers

Then you can load this model and run inference.

from sentence_transformers import SentenceTransformer

# Download from the 🤗 Hub
model = SentenceTransformer("jiwonyou0420/encoder-qa-finetuned")
# Run inference
sentences = [
    'What is the Schwarzschild radius and how is it related to black holes? Calculate the Schwarzschild radius for a black hole with a mass of 5 solar masses.',
    'microlensing events, such as those conducted by the macho, eros, and ogle projects, have placed constraints on the abundance of pbhs in the mass range of 10 ^ ( - 7 ) to 1 m☉. while these constraints rule out pbhs as the dominant form of dark matter in this mass range, they do not exclude the possibility of a subdominant population. 2. cosmic microwave background ( cmb ) radiation : the presence of pbhs during the early universe could have affected the cmb radiation. current cmb data from the planck satellite has placed constraints on the abundance of pbh',
    'of electronic properties under strong magnetic fields, one can gain insights into the fermi surface and the presence of topologically protected states. in summary, the band structure of a topological insulator is characterized by a bulk bandgap and topologically protected surface or edge states that enable conducting behavior. these unique electronic properties can be experimentally observed and measured using techniques such as arpes, stm, and transport measurements.',
]
embeddings = model.encode(sentences)
print(embeddings.shape)
# [3, 384]

# Get the similarity scores for the embeddings
similarities = model.similarity(embeddings, embeddings)
print(similarities.shape)
# [3, 3]

Training Details

Training Dataset

Unnamed Dataset

• Size: 8,814 training samples
• Columns: sentence_0, sentence_1, and label
• Approximate statistics based on the first 1000 samples:

  	sentence_0	sentence_1	label
  type	string	string	float
  details	min: 16 tokens mean: 46.41 tokens max: 139 tokens	min: 3 tokens mean: 115.62 tokens max: 169 tokens	min: 0.0 mean: 0.52 max: 1.0

• Samples:

  sentence_0	sentence_1	label
  What is the minimum frequency of incident light required to cause the photoelectric effect on a potassium atom with a work function of 2.3 eV? Calculate the kinetic energy of the emitted photoelectron if the incident frequency is twice the minimum frequency.	and controlling pwi is essential for the development of efficient and long - lasting fusion reactors.	0.0
  How do non-perturbative gauge dynamics impact the predictions of string theory for high-energy particle interactions?	reflected = i _ incident - ( 1 / 2 ) i _ incident i _ reflected = ( 1 / 2 ) i _ incident so, the maximum possible reflection of polarized light when it passes through a polarizer whose transmission axis is at an angle of 45 degrees to the incident polarization is 50 % of the incident light intensity.	0.0
  What is the maximum mass that a star can have before it undergoes a supernova explosion, and what are the main nucleosynthesis processes that occur during the explosion?	the maximum mass that a star can have before it undergoes a supernova explosion is determined by the tolman - oppenheimer - volkoff ( tov ) limit. this limit is approximately 3 solar masses ( m☉ ) for neutron stars, which are the remnants of supernova explosions. however, the progenitor star ( the star before the supernova ) can have a much larger mass, typically between 8 to 20 solar masses or even higher, depending on various factors such as metallicity and rotation. there are two main types of supernova explosions : type ia and type ii. the nucleosynthesis processes that occur during	1.0

• Loss: CosineSimilarityLoss with these parameters:

  {
      "loss_fct": "torch.nn.modules.loss.MSELoss"
  }
  

Training Hyperparameters

Non-Default Hyperparameters

• per_device_train_batch_size: 4
• per_device_eval_batch_size: 4
• num_train_epochs: 1
• multi_dataset_batch_sampler: round_robin

All Hyperparameters

Click to expand

• overwrite_output_dir: False
• do_predict: False
• eval_strategy: no
• prediction_loss_only: True
• per_device_train_batch_size: 4
• per_device_eval_batch_size: 4
• per_gpu_train_batch_size: None
• per_gpu_eval_batch_size: None
• gradient_accumulation_steps: 1
• eval_accumulation_steps: None
• torch_empty_cache_steps: None
• learning_rate: 5e-05
• weight_decay: 0.0
• adam_beta1: 0.9
• adam_beta2: 0.999
• adam_epsilon: 1e-08
• max_grad_norm: 1
• num_train_epochs: 1
• max_steps: -1
• lr_scheduler_type: linear
• lr_scheduler_kwargs: {}
• warmup_ratio: 0.0
• warmup_steps: 0
• log_level: passive
• log_level_replica: warning
• log_on_each_node: True
• logging_nan_inf_filter: True
• save_safetensors: True
• save_on_each_node: False
• save_only_model: False
• restore_callback_states_from_checkpoint: False
• no_cuda: False
• use_cpu: False
• use_mps_device: False
• seed: 42
• data_seed: None
• jit_mode_eval: False
• use_ipex: False
• bf16: False
• fp16: False
• fp16_opt_level: O1
• half_precision_backend: auto
• bf16_full_eval: False
• fp16_full_eval: False
• tf32: None
• local_rank: 0
• ddp_backend: None
• tpu_num_cores: None
• tpu_metrics_debug: False
• debug: []
• dataloader_drop_last: False
• dataloader_num_workers: 0
• dataloader_prefetch_factor: None
• past_index: -1
• disable_tqdm: False
• remove_unused_columns: True
• label_names: None
• load_best_model_at_end: False
• ignore_data_skip: False
• fsdp: []
• fsdp_min_num_params: 0
• fsdp_config: {'min_num_params': 0, 'xla': False, 'xla_fsdp_v2': False, 'xla_fsdp_grad_ckpt': False}
• tp_size: 0
• fsdp_transformer_layer_cls_to_wrap: None
• accelerator_config: {'split_batches': False, 'dispatch_batches': None, 'even_batches': True, 'use_seedable_sampler': True, 'non_blocking': False, 'gradient_accumulation_kwargs': None}
• deepspeed: None
• label_smoothing_factor: 0.0
• optim: adamw_torch
• optim_args: None
• adafactor: False
• group_by_length: False
• length_column_name: length
• ddp_find_unused_parameters: None
• ddp_bucket_cap_mb: None
• ddp_broadcast_buffers: False
• dataloader_pin_memory: True
• dataloader_persistent_workers: False
• skip_memory_metrics: True
• use_legacy_prediction_loop: False
• push_to_hub: False
• resume_from_checkpoint: None
• hub_model_id: None
• hub_strategy: every_save
• hub_private_repo: None
• hub_always_push: False
• gradient_checkpointing: False
• gradient_checkpointing_kwargs: None
• include_inputs_for_metrics: False
• include_for_metrics: []
• eval_do_concat_batches: True
• fp16_backend: auto
• push_to_hub_model_id: None
• push_to_hub_organization: None
• mp_parameters:
• auto_find_batch_size: False
• full_determinism: False
• torchdynamo: None
• ray_scope: last
• ddp_timeout: 1800
• torch_compile: False
• torch_compile_backend: None
• torch_compile_mode: None
• include_tokens_per_second: False
• include_num_input_tokens_seen: False
• neftune_noise_alpha: None
• optim_target_modules: None
• batch_eval_metrics: False
• eval_on_start: False
• use_liger_kernel: False
• eval_use_gather_object: False
• average_tokens_across_devices: False
• prompts: None
• batch_sampler: batch_sampler
• multi_dataset_batch_sampler: round_robin

Training Logs

Epoch	Step	Training Loss
0.2269	500	0.0759
0.4537	1000	0.0546
0.6806	1500	0.0528
0.9074	2000	0.0465

Framework Versions

• Python: 3.12.8
• Sentence Transformers: 3.4.1
• Transformers: 4.51.3
• PyTorch: 2.5.1+cu124
• Accelerate: 1.3.0
• Datasets: 3.2.0
• Tokenizers: 0.21.0

Citation

BibTeX

Sentence Transformers

@inproceedings{reimers-2019-sentence-bert,
    title = "Sentence-BERT: Sentence Embeddings using Siamese BERT-Networks",
    author = "Reimers, Nils and Gurevych, Iryna",
    booktitle = "Proceedings of the 2019 Conference on Empirical Methods in Natural Language Processing",
    month = "11",
    year = "2019",
    publisher = "Association for Computational Linguistics",
    url = "https://arxiv.org/abs/1908.10084",
}