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A rise and fall behaviour of the multiplicity of intermediate mass fragments (IMFs) is observed. The system size dependence of peak center-of-mass energy E$_{c.m.} ^{max}$ and peak IMF multiplicity $<$N$_{IMF}>^{max}$ is also studied, where it is observed that E$_{c.m.}^{max}$ fol"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1106.1537","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2011-06-08T11:00:33Z","cross_cats_sorted":[],"title_canon_sha256":"742512542b956bd1f503b43e6d3d190a640c16a5293db266cd32b655d791bb13","abstract_canon_sha256":"c75f325419b4615e5fe53ab764cf1060a941a6bfc03824165b32acf48d1306ea"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:20:22.811850Z","signature_b64":"USuV4ByRtcGAQx311pejKreTt3aYLPXFShmHf1+jUwbo+xnhrXwXFeYCxwLpdf5t2qSDnSl7qeWRc7bJVzGPCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cd9947dd6a7890ca0b7809b6ba7e3ed755cccd5ca04d03251fdd4bac83a4c973","last_reissued_at":"2026-05-18T04:20:22.811280Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:20:22.811280Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"System size dependence of intermediate mass fragments in heavy-ion collisions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"Sukhjit Kaur","submitted_at":"2011-06-08T11:00:33Z","abstract_excerpt":"We simulate the central reactions of $^{20}$Ne+$^{20}$Ne, $^{40}$Ar+$^{45}$Sc, $^{58}$Ni+$^{58}$Ni, $^{86}$Kr+$^{93}$Nb, $^{129}$Xe+$^{118}$Sn, $^{86}$Kr+$^{197}$Au and $^{197}$Au+$^{197}$Au at different incident energies for different equations of state (EOS), binary cross sections and different widths of Gaussians. 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